Posts Tagged ‘Nasa’

Inside NASA’s world-class supercomputer center

April 26th, 2010

MOUNTAIN VIEW, Calif.–If you’re a materials scientist at NASA’s Glenn Research Center, or an engineer at the Johnson or Marshall Space Centers studying Space Shuttle flow-control valves, or any one of countless others in the agency needing a supercomputer, there’s really just one place to go.That place is the advanced supercomputing facility at the Ames Research Center here, the home of Pleiades, NASA’s flagship computer, a monster of a machine that, with a current rating of 973 teraflops–or 973 trillion floating point operations per second–is today ranked the sixth-most powerful supercomputer on Earth.The computing facility, which services about 1,500 users across NASA, according to Rupak Biswas, the agency’s advanced supercomputing division chief, is somewhat of a one-stop shop for those needing the highest-end processing power NASA has to offer: the division provides not just computing power, but also a “fully integrated environment where people have access to the machine, and [where] we assist them to get the most out of the machine.”Pleiades, like most, if not all, supercomputers, is a work in progress. Debuted in late 2008 with a world No. 3 ranking and a measurement of 487 teraflops, the machine how now doubled its capacity, even as it has dropped three places in the rankings. Based on SGI’s Altix ICE system, Pleiades still has room to grow, and as Biswas and his staff at the supercomputing division add more SGI racks, it will do just that.
And that’s vital to NASA because the demands for the computer’s use are non-stop. Across the agency, Biswas must support anyone granted time on the computer, be it for doing climate modeling, researching weather patterns caused by El Nino, understanding how galaxies merge or investigating the next generation of space vehicles.

Twenty-five-plus years of NASA supercomputing Last week, I got a chance to visit Biswas and see Pleiades up close. Biswas explained that he and his staff work 24 hours a day, seven days a week servicing the demands for time on Pleiades and the other machines under his command, making sure to offer NASA’s scientists support for application performance optimization, data analysis and visualization and networking. Essentially, though, the supercomputers are used for a never-ending supply of modeling and simulation tasks, and Biswas said that just about every available computer cycle that the division’s machines have to offer are spoken for.Inside NASA’s world-class supercomputer center (photos) While NASA has offered its people high-end computers for years, the agency changed its model in 1984, when it opened the doors of the advanced supercomputing facility and began focusing on providing “leading-edge computational capabilities based on an innovative network-centric environment,” according to a 2008 brochure celebrating the 25th anniversary of the division.Things have come a very long way since then. The division’s first supercomputer, the Cray X-MP, was measured at 0.00021 teraflops–or as the brochure puts it today, less power than a single Apple Mac Mini personal computer. But over the years, supercomputers in general have outperformed Moore’s Law, Biswas told me, because they are made up of the very latest equipment and processors.

In 2003, the Space Shuttle Columbia exploded, and NASA went into full-scale investigation mode, trying to determine what caused the disaster, and that became one of the primary motivations for rolling out what came to be known as the Columbia supercomputer in 2004.But that wasn’t the only driving factor, he said. There also was a touch of national competitiveness. Indeed, Biswas said, despite the fact that most Americans thought the Japanese were bluffing, computer scientists in Japan managed to build the Earth Simulator, which was the fastest supercomputer in the world. That caused, Biswas recalled, “a lot of panic in the U.S.” as people thought “we are losing leadership in high-end computing.”By the time Columbia debuted in 2004, Japan had been surpassed, not just by the new NASA supercomputer–which came in at No. 2 in the world–but also by a new machine at Lawrence Livermore National Laboratory, which was the fastest on the planet. By then, the Earth Simulator had dropped off the very top of the leader board.

Supercomputers are like most other class of machine: they have limited lifespans–in their case, about three years. After that, Biswas said, “it’s not cost-effective to run them anymore.That’s in part because advances are happening in the industry so fast that after that time period, new technologies have far surpassed what was once cutting-edge. Further, the industry moves quickly in figuring out new ways to package supercomputers, meaning they require much less power than older models. “Supercomputers advance so rapidly,” Biswas said, it “does not makes sense from an economic standpoint to run old supercomputers.”During a three-year cycle, supercomputer divisions will typically look at what’s new that’s out there, take in proposals from the different vendors, and then procure a small test-bed, Biswas explained. After “kicking the tires” on a new machine, and seeing how it works in an existing supercomputing environment, and how well it can support those who would be using it, a division like that at NASA will make a decision on which new supercomputer to purchase.Prior to purchasing the SGI equipment that makes up Pleiades, the NASA supercomputing division purchased an IBM p575+ supercomputer in order to evaluate it. Eventually, the division decided on the SGI approach, but the IBM equipment is still in the supercomputing facility at Ames, and today operates under the name Schirra, named after the Mercury 7 astronaut Wally Schirra.The move to exaflop supercomputers Today, the world’s fastest supercomputers are topping out at about 1 petaflop–or 1,000 trillion floating point operations per second. Biswas said there are about five such computers on Earth today, two at the LINK Oak Ridge National Lab in Tennessee, one in China, and one in Germany. And Pleiades is just behind that. But already, he said, the next-generation thinking in the industry is envisioning machines capable of exaflop computing, which is the equivalent of 1,000 petaflops. Of course, as with any new supercomputing threshold, the question isn’t necessarily whether it’s possible to build the hardware, but whether it’s also possible to optimize applications for such a powerful system. And not only that, Biswas said, but there’s also a crucial question of whether it’s possible to build machines that powerful and yet have them be energy efficient.

A petaflop supercomputer draws about 7 megawatts of power, he explained. That would mean that without increased efficiencies, an exaflop machine would draw 7 gigawatts. And that’s simply out of the question. “You can’t expect to have a nuclear reactor sitting next to a supercomputer,” he said.The bigger question would be, what will the right applications be for computers that could be 1,000 times or more faster than today’s top-end, and which could potentially reach that strength by 2018. There’s no point in building such machines, Biswas suggested, unless they’re being used at peak efficiency.
At NASA, one use case could be to try to, finally, accurately predict weather. “Today, forget about predicting weather five days from now,” Biswas said. “You can’t even do today.”

And the reason, he explained, is that even with today’s massively powerful computers, it’s not possible to create models fine enough to distill weather forecasts at the kind of small resolution necessary to be correct and relevant and timely. But with a thousand-fold boost in supercomputing juice, it could theoretically happen at that resolution.Another use of an exaflop supercomputer would be to do richer modeling of the relationship between the Earth’s atmosphere and our oceans. And that relationship must be coupled with what’s taking place on terra firma. And then add in what’s going on at the polar ice caps, and you have, as Biswas put it, “a huge, complex calculation” that cannot be done today. “That requires exaflop” computing.

Being NASA, of course, there’s also plenty of applications for rocket science. Biswas said engineers wanting a complete digital model of a launch could find ample uses for an exaflop supercomputer. Today, he said, it is possible to model the first few seconds of a Shuttle launch, but to be able to put together a full profile, from launch to stage separation to an entire mission, “that’s easily a multi-exaflop” problem.And marrying the idea of weather forecasting with launch analysis, such computers may also for the first time allow NASA to make better decisions surrounding when it’s safe to launch. “Right now, NASA launches by looking at the weather forecast,” Biswas said. “If it’s not good, [don't] launch. Ultimately, you want to couple the weather with the launch.”

Source:-http://news.cnet.com/8301-13772_3-20003333-52.html

NASA engineers join toyota investigation

March 31st, 2010

Transportation Secretary Ray LaHood is bringing in a team of nine NASA engineers who specialize in computer-controlled electronic systems, electromagnetic interference, software integrity and hardware to help his department investigate alleged unintended vehicle acceleration in Toyota vehicles.

Transportation also is commissioning a separate investigation from the National Academy of Sciences, according to a news release of March 30. “For the safety of the American driving public, we must do everything possible to understand what is happening. And that is why we are tapping the best minds around, LaHood said.”

The National Academy of Sciences will examine the broad subject of unintended acceleration and electronic vehicle controls across the entire automotive industry. The investigation is expected to take 15 months.

The academy’s panel of experts will examine possible causes of the unintended acceleration, including electronic vehicle controls, human error, mechanical failure and interference with accelerator systems. Systems to be examined include software, computer hardware design, electromagnetic compatibility and electromagnetic interference. The panel will make recommendations on how its regulations may improve safety in electronic control systems.

The cost of the two studies is approximately $3 million, including the cost of purchasing affected cars to be studied, the news release said.

LaHood has also asked Transportation’s inspector general to review whether the department has conducted adequate reviews of unintended acceleration complaints since 2002

Source:-http://fcw.com/articles/2010/03/31/dot-enlisting-nasa-engineers-for-toyota-investigation.aspx

NASA to help probe unintended auto acceleration

March 30th, 2010

The U.S. Transportation Department will launch two major investigations to discover whether vehicle electronics or electromagnetic interference are to blame for unintended vehicle acceleration incidents.

The investigations, one by the National Academy of Sciences and the other with the help of the NASA, will help get to the bottom of the issue, U.S. Transportation Secretary Ray LaHood said in an interview with The Detroit News Monday.
The announcement follows congressional hearings in recent months into reports of hundreds of runaway Toyota Motor Corp. vehicles.

LaHood said the investigation will not be limited to Toyota, but will cover all manufacturers.

Toyota has recalled 8.5 million vehicles worldwide over concerns of runaway vehicles. The National Highway Traffic Safety Administration, an agency of the transportation department, has received more than 3,000 complaints — that include at least 51 deaths since 2000 — linked to runaway Toyotas.

The Japanese automaker says it does not believe electronics or electromagnetic interference is the cause. It blames entrapped or malfunctioning pedals.

“Many members of Congress think it’s electronics and I heard enough of that — not only from members but from Toyota drivers … and so we felt we really needed to get outside experts,” LaHood said. “We are tapping the best minds around.”

Toyota welcomed the investigation by the National Academy of Sciences and NASA.

“We expect they will bring a thorough and scientific approach to their examination of the issues. Separating fact from fiction can only be good for the motoring public and the industry as a whole,” the company said in a statement late Monday.

“We are confident in our vehicles and in our electronics. We will lend our full support and cooperation to DOT and NHTSA as they moved forward.”

Probe to last 15 months

LaHood also is asking the U.S. Department of Transportation Inspector General to review whether NHTSA’s Office of Defect Investigation has the necessary resources and systems to identify and address safety defects in the nation’s automobiles.

LaHood said he wasn’t ready to blame electronics, but noted that modern cars depend heavily on computers.

“The cars that are being manufactured today are primarily computers,” LaHood said. “I’ve listened to enough people who believe that electronics is a problem that we just have to find that out.”

LaHood said the National Academy of Sciences, an independent body using top scientific experts, will “examine the broad subject of unintended acceleration and electronic vehicle controls across the entire automotive industry.” The examination will occur over the course of 15 months.

Experts will review industry and government efforts to identify possible sources of unintended acceleration, including electronic vehicle controls, human error, mechanical failure and interference with accelerator systems.

The Academy “has an impeccable reputation that we just felt if we could persuade them to get involved in this it would lend a lot of credibility to whatever they have say,” LaHood said.

NASA scientists involved

Separately, he said, NHTSA has enlisted NASA scientists with expertise in areas such as computer-controlled electronic systems, electromagnetic interference and software integrity to help investigate the issue of unintended vehicle acceleration in Toyota vehicles.

“For the safety of the American driving public, we must do everything possible to understand what is happening. And that is why,” LaHood said.

The experts will look at software, computer hardware design, electromagnetic compatibility and electromagnetic interference.
They will make recommendations to NHTSA on how its rulemaking, research and defect investigation activities may help ensure the safety of electronic control systems in motor vehicles.

The NHTSA review of the electronic throttle control systems in Toyotas will be completed by late summer.
NHTSA has brought in NASA engineers and other experts in subjects such as electromagnetic compatibility as part of a shorter-term review of the systems used in Toyota vehicles to determine whether they contain any possible flaws that would warrant a defect investigation.

LaHood said the department will spend $3 million on the two studies, including the cost of purchasing cars that have allegedly experienced unintended acceleration for inspection.

Source:http://detnews.com/article/20100330/AUTO01/3300329/NASA-to-help-probe-unintended-auto-acceleration

NASA will help probe Toyota acceleration problem

March 30th, 2010

NASA and the National Academy of Sciences are joining the government’s effort to figure out what caused the sudden acceleration problems that led to Toyota’s massive recalls.

NASA scientists with expertise in electronics will help the National Highway Traffic Safety Administration study potential electronic ties to unintended acceleration in Toyotas. NASA’s knowledge of electronics, computer hardware and software and hazard analysis will ensure a comprehensive review, Transportation Secretary Ray LaHood said Monday.

In a separate study, the National Academy of Sciences will examine unwanted acceleration and electronic vehicle controls in cars from around the auto industry, LaHood said. The National Academy is an independent organization chartered by Congress.

The academy study, expected to take 15 months, will review acceleration problems and recommend how the government can ensure the safety of vehicle electronic control systems.

“We believe their outside expertise, fresh eyes and fresh research perhaps can tell us if electronics have played a role in these accelerations,” LaHood said.

Source:http://www.forbes.com/feeds/ap/2010/03/29/general-us-toyota-recall_7473691.html

NASA ISS On-Orbit Status

March 30th, 2010

All ISS systems continue to function nominally, except those noted previously or below. Underway: Week 2 of Increment 23. (Day 99 in space for Oleg Kotov, Timothy Creamer & Soichi Noguchi). >>>Today in 1974, NASA’s Mariner 10 became the first space probe to fly by the Planet Mercury, after launch on 11/3/73.<<<

At wake-up, CDR Oleg Kotov performed the regular daily early-morning check of the aerosol filters at the Russian Elektron O2 generator which Maxim Suraev had installed on 10/19 in gaps between the BZh Liquid Unit and the oxygen outlet pipe (filter FA-K) plus hydrogen outlet pipe (filter FA-V). [CDR again inspected the filters before bedtime this morning, currently a daily requirement per plan, with photographs to be taken if the filter packing is discolored.]

Kotov’s morning inspection today included the weekly checkup behind ASU/toilet panel 139 in the SM (Service Module) on a fluid connector (MNR-NS) of the SM-U urine collection system, looking for potential moisture.

Working in the COL (Columbus Orbital Laboratory), FE-5 Noguchi prepared rack bay F3 as part of outfitting for the arrival of a new ISPR (International Standard Payload Rack) with the ESA MARES (Muscle Atrophy Research & Exercise System) payload on 19A. [Preparatory activities involved ISPR bonding strap installation, installation of the right & left K-Bar capture mechanisms on the overhead forward standoff, and installation of left & right pivot pin brackets, followed by cleaning out the F3 bay by relocating NASA & ESA CTBs (Cargo Transfer Bags) and other items. MARES will be used for research on musculoskeletal, biomechanical, and neuromuscular human physiology to better understand the effects of microgravity on the muscular system. The payload consists of an adjustable chair & human restraint system, a pantograph (an articulated arm supporting the chair, used to properly position the user), a direct drive motor, associated electronics & experiment programming software, a linear adapter that translates motor rotation into linear movements, and a vibration isolation frame. MARES may also be used in conjunction with the associated PEMS II (Percutaneous Electrical Muscle Stimulator) device. MARES enables scientists to study the detailed effects of microgravity on the human muscle-skeletal system and also provides a means to evaluate countermeasures designed to mitigate the negative effect, especially muscle atrophy, supporting measurements and exercise on seven different human joints, encompassing nine different angular movements, as well as two additional linear movements (arms and legs). The system is considerably more advanced than current ground-based medical dynamometers (devices used to measure force or torque) and a vast improvement over existing ISS muscle research facilities.]

Afterwards, Noguchi moved to the “Destiny” Lab to clean out its D3 bay in similar preparation for the arrival of the WORF (Window Observational Research Facility) rack on 19A. [Stowed payload hardware was relocated from D3 to the Kibo JPM (JEM Pressurized Module)’s A4 rack front. WORF, designed for the high-quality Lab science window, is based on an ISPR, utilizing avionics & hardware adapted from the ER (EXPRESS Rack) program. With a payload volume equivalent to 0.8 m3, the rack can support up to three payloads simultaneously, depending on available resources and space available at the window. WORF will also provide access & equipment for crew Earth observations, such as crew restraints, camera/camcorder brackets and condensation prevention. Its payloads will focus on geology, agriculture, ranching, environmental & coastal changes, and education.]

Later, Soichi spent an additional hour on general stowage cleanup, consolidating & relocating NASA hardware to make room for new payloads items arriving on 19A, removing cargo for MPLM (Multi-Purpose Logistics Module) docking, and clearing hatchways.

Working in the Progress M-04M/36P cargo ship docked at the SM aft port, Kotov had ~4.5 hrs to dismantle the KURS-A hardware and remove it in its container, to be recycled on a later flight.

The CDR also performed periodic service of the RS (Russian Segment) radiation payload suite “Matryoshka-R” (RBO-3-2), recording data from detectors in the Bubble-dosimeter reader and rearranging some dosimeters. [Eight Bubble dosimeter detectors (A01-A08) are positioned at their exposure locations around the RS. An additional eight detectors were placed by Maxim at the spherical “Phantom” unit in the DC1 Docking Compartment. The deployment locations of the detectors and their measurements reported to TsUP via log sheet over OCA. The complex Matryoshka payload suite is designed for sophisticated radiation studies. Note: Matryoshka is the name for the traditional Russian set of nested dolls.]

Later, Oleg completely deactivated the running BIO-5 Rasteniya-2 ("Plants-2") experiment in the SM. [Rasteniya-2 researches growth and development of plants under spaceflight conditions in the LADA-16 greenhouse from IBMP (Institute of Bio-Medical Problems, Russian: IMBP), currently planted with Mizuna seeds. Mizuna (Brassica rapa nipposinica) is a tasty variety of Japanese mustard greens, also known as California Peppergrass, eaten as a salad.]

FE-6 Creamer worked in the US A/L (Airlock), unstowing and preparing equipment for the upcoming 19A spacewalks. [Activities included removing any unused hardware from the A/L, pregathering three EMU (Extravehicular Mobility Unit) cuff checklists, removing the third SAFER (Simplified Aid For EVA Rescue) unit and PHA (Prebreathe Hose Assembly) spares kit from the A/L, cleaning out EMU equipment bag EV1 & EV2 compartments, etc.]

Also in the A/L, FE-5 Noguchi later initiated another recharge on REBA (Rechargeable EVA Battery Assembly) #1006 which did not receive a nominal charge during last week’s battery charging event (3/24). [It is hoped that the second attempt will acquire more technical data to allow specialists to evaluate the charging anomaly.]

In Node 2, FE-6 cleaned the inlet of the forward starboard IMV (Intermodule Ventilation) fan ducting.

Afterwards, Timothy conducted the regular 30-day inspection of the AED (Automated External Defibrillator) in the CHeCS (Crew Health Care Systems) rack. [The AED is a portable electronic device that automatically diagnoses the potentially life threatening cardiac arrhythmias of ventricular fibrillation and ventricular tachycardia in a patient. It then can treat them through defibrillation, i.e., the application of electrical therapy which stops the arrhythmia, allowing the heart to re-establish an effective rhythm. AEDs are generally either held by trained personnel who will attend events or are public access units which can be found in places including corporate and government offices, shopping centers, airports, restaurants, casinos, hotels, sports stadiums, schools and universities, community centers, fitness centers, health clubs and any other location where people may congregate.]

Creamer also performed maintenance on the PWD (Potable Water Dispenser), -
Removing & replacing its beverage adapter (modified with only one fastener instead of two),
Removing & replacing the PWD needle (using a new design that helps prevent backflow and leakage), and
Photo-documenting the PWD standoff hose for an inspection of its chafing protection.

Oleg & TJ reviewed instructional video material to refresh their RPM (R-bar Pitch Maneuver) ops proficiency and then tagged up with ground specialists at ~11:30am EDT to discuss photo/video procedures. [The RPM flip-over is used by the crew for the bottom-side mapping of the Orbiter at the arrival of the Shuttle at 4/7. During the RPM at ~600 ft from the station, the “shooters” have only ~90 seconds for taking high-resolution digital photographs of all tile areas and door seals on Discovery, to be downlinked for launch debris assessment. Thus, time available for the shooting will be very limited, requiring great coordination between the two headset-equipped photographers and the Shuttle pilot.]

Noguchi initiated (later terminated) another 5-hr sampling run (the 81st) with the EHS GC/DMS (Environmental Health System Gas Chromatograph/Differential Mobility Spectrometer). [Also known as AQM (Air Quality Monitor), the system is controlled with “Sionex” expert software from the SSC-12 laptop. The AQM demonstrates COTS (Commercial Off-the-Shelf) technology for identifying volatile organic compounds, similar to the VOA (Volatile Organics Analyzer). This evaluation will continue over the course of several months as it helps to eventually certify the GC/DMS as nominal CHeCS (Crew Health Care Systems) hardware.]

On the CIR (Combustion Integrated Rack) in the Lab, Soichi removed the alignment guides to allow activation of the PaRIS (Passive Rack Isolation System) by the ground for FCF (Fluids & Combustion Facility) operations requiring a microgravity environment.

Oleg Kotov completed the routine daily servicing of the SOZh system (Environment Control & Life Support System, ECLSS). [Regular daily SOZh maintenance consists, among else, of checking the ASU toilet facilities, replacement of the KTO & KBO solid waste containers and replacement of EDV-SV waste water and EDV-U urine containers.]

The crew completed their regular daily 2.5-hr. physical workout program on the ARED advanced resistive exerciser (FE-5, FE-6), T2/COLBERT advanced treadmill (CDR, FE-5, FE-6), and VELO ergometer bike with bungee cord load trainer (CDR).

At ~10:30am EDT, TJ Creamer & Soichi Noguchi supported a PAO TV interview with WJZ-TV/Channel 13 in Baltimore (TJ is from Upper Marlboro, MD), and downlinked two messages of greetings and well-wishing for ESA, one for the annual Madrid, Spain, Campus Party of thousands of participants in a range of different activities related to computers, communications and new technologies, the second for the annual Berlin Air Show’s Parliamentarians’ Day in the ESA/DLR Pavilion on June 11.

At ~10:58am, Soichi powered up the SM's amateur radio equipment (Kenwood VHF transceiver with manual frequency selection, headset, & power supply) and at 11:03am conducted a ham radio session with students at Walnut Creek Elementary School in Azle, TX, USA.

Noguchi powered down the TVIS (Treadmill with Vibration Isolation & Stabilization) by opening its two 20 amp circuit breakers at SM panel 435 in preparation for tomorrow’s scheduled repair of the broken exercise machine.

FE-5 & FE-6 are scheduled for their periodic PMC (Private Medical Conferences), via S- & Ku-band audio/video, Creamer at ~1:35pm, Noguchi at ~2:00pm.

Soichi & TJ will also have their weekly PFCs (Private Family Conferences), both at ~5:30pm before sleeptime.

Jobs listed for Oleg for today on the Russian discretionary “as time permits” task list were –
The daily IMS (Inventory Management System) maintenance, updating/editing its standard “delta file” including stowage locations, for the regular weekly automated export/import to its three databases on the ground (Houston, Moscow, Baikonur), and
Another video shoot with the SONY HVR-Z7U camcorder of Lake Baikal. [Roskosmos TV studio is working on a feature on Lake Baikal and its importance as natural heritage, called ‘Planet Baikal’. The feature will be broadcast in Vesti channel’s weekly program Kosmonavtika. The Baikal Lake contains 20% of the world’s water reserves; it is a beautiful and a mysterious lake. The producers want to highlight the grandeur of this natural gem and raise awareness about its pollution problems. The metaphor used throughout the feature is one of a planet, an element of the Universe and a cosmonaut talking about Baikal while on orbit is thought to be a perfect choice to convey it. The feature item will be filmed and broadcast to Earth in real time later (April 6-9).]

No CEO photo targets uplinked for today.

WPA Update: The Water Processor Assembly is still down. Suspected location of the leak is in the area around the catalytic reactor. Rack rotation and inspection of the reactor by the crew is scheduled tomorrow. The reactor’s thermal cover has 12 non-captive fasteners and washers to be removed. If the reactor turns out to be defect, a new spare will be flown up in 19A. Also, a connector will be changed to allow processing using the UPA (Urine Processor Assembly) and returning the current RFTA (Recycle Filter Tank Assembly on 19A, plus mitigating the number of EDVs used. The crew is currently using Russian drinking water, through 19A.

Source:-http://www.spaceref.com/news/viewsr.html?pid=33785

Nasa isss on-orbit status 26 March 2010

March 26th, 2010

All ISS systems continue to function nominally, except those noted previously or below.

At wake-up, CDR Oleg Kotov performed the regular daily early-morning check of the aerosol filters at the Russian Elektron O2 generator which Maxim Suraev had installed on 10/19 in gaps between the BZh Liquid Unit and the oxygen outlet pipe (filter FA-K) plus hydrogen outlet pipe (filter FA-V). [CDR again inspected the filters before bedtime this morning, currently a daily requirement per plan, with photographs to be taken if the filter packing is discolored.]

FE-6 Creamer continued the new week-long session of experiment SLEEP (Sleep-Wake Actigraphy & Light Exposure during Spaceflight), TJ’s third, transferring data from his Actiwatch to the HRF-1 (Human Research Facility 1) laptop. [To monitor his/her sleep/wake patterns and light exposure, the crewmember wears a special Actiwatch device which measures the light levels encountered by him/her as well as their patterns of sleep and activity throughout the Expedition, using the payload software for data logging and filling in questionnaire entries in the experiment’s laptop session file on the HRF-1 laptop. The log entries are done within 15 minutes of final awakening for seven consecutive days.]

Soichi Noguchi & Timothy Creamer completed another Reaction Self Test (Psychomotor Vigilance Self Test on the ISS) protocol. [The RST is performed twice daily (after wakeup & before bedtime) for 3 days prior to the sleep shift, the day(s) of the sleep shift and 5 days following a sleep shift. Originally planned for a total of 121 RST runs, Jeff completed 108 runs by the time of his return last week. The experiment consists of a 5-minute reaction time task that allows crewmembers to monitor the daily effects of fatigue on performance while on ISS. The experiment provides objective feedback on neurobehavioral changes in attention, psychomotor speed, state stability, and impulsivity while on ISS missions, particularly as they relate to changes in circadian rhythms, sleep restrictions, and extended work shifts.]

The crew performed the mandatory 1h 20m OBT (onboard training) Depress Emergency drill for the case of rapid cabin depressurization, with Russian & US specialists standing by at both control centers for crew questions or comments, followed by a 10-min debrief with ground specialists. The crew practiced ISS depress response procedures, coordination between themselves during the depress, and coordination with Mission Control Centers during the depress as well as on emergency egress from the ISS. [Background: Purpose of the drill is to (a) familiarize the station residents with the location of hardware and the positions of valves used in emergency situations, (b) perform a survey of each hatch for drag-through cables (and reporting results to MCC), (c) work through the RS (Russian Segment) hardware deactivation procedures, (c) practice crew emergency joint activities, and (d) identify crew comments and suggestions that arise during training regarding crew procedures and equipment. In the RS, the crew usually translates along the emergency egress paths to the FGB nadir port (where Soyuz 21S is currently docked), checking hardware such as the Sokol suits, cable cutters, fire extinguisher (OKR), gas masks (IPK), emergency procedures books, valve settings, hatch rubber seal & restraint integrity, etc. In the US Segment (USOS) the inspection usually focuses on readiness of CSA-CP (Compound Specific Analyzer-Combustion Products), ISS leak kit, PBA (portable breathing assembly) and PFE (portable fire extinguisher), emergency procedures books, valve settings, integrity of hatch rubber seals, presence of hatch handrails, etc. The checks also include Node-3, Node-2, COL (Columbus Orbital Laboratory), JLP (Japanese Experiment Module Experiment Logistics Module Pressurized Section) and Kibo JPM (JEM Pressurized Module). The exercise was topped off by a debrief with the ground via S-band. During the session, the crew simulated executing the planned emergency procedures while moving about the station. For the case of an onboard fire and for emergency descent, there are other mandatory emergency drill OBTs.]

Working on the BSA (Battery Stowage Assembly) in the US A/L (Airlock), Noguchi terminated EMU (Extravehicular Mobility Unit) battery recharging.

Later, FE-5 prepared three PGTs (Pistol Grip Tools) for the 19A spacewalks, installing batteries in the units (#1004 in PGT-6, #1006 in PGT-2, #1005 in PGT-1) and checking out the devices, leaving the batteries installed when finished.

Also for the EVAs, Soichi checked out two SAFER units (Simplified Aid For EVA Rescue), – #1005 & #1006.

Creamer supported the ground in trying to retrieve missing data files from an exercise workout on 3/21 on the T2 treadmill, that were transferred by FE-6 to an SSC (Station Support Computer) but not recovered by the ground.

TJ & Soichi filled out their weekly FFQs (Food Frequency Questionnaires) on the MEC (Medical Equipment Computer). [On the FFQs, NASA astronauts keep a personalized log of their nutritional intake over time on special MEC software. Recorded are the amounts consumed during the past week of such food items as beverages, cereals, grains, eggs, breads, snacks, sweets, fruit, beans, soup, vegetables, dairy, fish, meat, chicken, sauces & spreads, and vitamins. The FFQ is performed once a week to estimate nutrient intake from the previous week and to give recommendations to ground specialists that help maintain optimal crew health. Weekly estimation has been verified to be reliable enough that nutrients do not need to be tracked daily.]

Soichi performed routine service on the prime CSA-CP (Compound Specific Analyzer-Combustion Products, #1042), replacing its battery with a new one (#1175).

CDR Kotov unstowed the equipment of the Russian DZZ-13 RUSALKA (“Mermaid”) science payload, set it up with its AIP-01 power supply and then conducted a test of the synchronization cable connecting it to the NIKON D2X digital camera. The setup was photo-recorded with a second NIKON, and the activity was supported by ground specialist tagup. [RUSALKA research relates to the Sun and the Earth's limb at sunset (atmosphere lighted), testing a procedure for remote determination of Methane (CH4) & Carbon Dioxide (CO2) content in the atmosphere (in the First Phase), measurement of CH4 & CO2 content in the atmosphere and reception of data on NI2 and NI4 content over the territories subjected to natural and technogenic effects, reception of sufficient data on seasonal dependencies of tropospheric parameters being studied (in the Second Phase). Equipment used: Rusalka monoblock, NIKON D2X(s) digital photo camera; AF VR Nikkor ED 80-400f/4.5-5.6D lens with ultraviolet filter, bracket for attachment to the window, and Rusalka-Accessories set. Support hardware: Device TIUS /DKShG/PNSK, Laptop RSK1, and Software Package loading disk.]

On the MSL (Materials Science Laboratory), Creamer performed sample exchange #6, removing yesterday’s CETSOL-1 sample from the SCA (Sample Cartridge Assembly) and replacing it with a new sample (MICAST-1). [The ESA/NASA MSRR-1 (Material Science Research Rack 1) provides a powerful multi-user MSL with diverse EMs (Experiment Modules) so that many material types, such as metals, alloys, polymers, semiconductors, ceramics, crystals, and glasses, can be studied in micro-G to discover new applications for existing materials and new or improved materials. MSRR experiments are coordinated by international teams that share different parts of the samples. There are 25 investigators on three research teams participating in the first of these investigations. CETSOL (Columnar-to-Equiaxed Transition in Solidification Processing) and MICAST (Microstructure Formation in Casting of Technical Alloys under Diffusive & Magnetically Controlled Convective Conditions) are two complementary material science projects to carry out research into the formation of microstructures during the solidification of metallic alloys. The goal of MICAST is to study the formation of microstructures during casting of technical alloys. In space, buoyancy convection is eliminated and the dendritic solidification of the alloys can be quantitatively studied under purely diffusive conditions. The objective of CETSOL is then to study the transition from columnar growth to equiaxed growth that occurs when crystals start to nucleate in the melt and grow independently. Results of these experiments will help to optimize industrial casting processes.]

TJ also salvaged all foam windscreens from discarded acoustic dosimeters stowed in an SMK (Sound Measurement Kit) slated to be returned to Earth on the 19A MPLM (Multi-Purpose Logistics Module). [One windscreen will be used on a new dosimeter (#1012) that’s missing its screen; the others will be stowed in the new SMK as spares.]

In the SM (Service Module), Oleg dismantled & removed the hardware of the GFI-1 “Relaksatsiya” (Relaxation) Earth Observation experiment at window #9, closing out the activity and stowing the equipment. [Using the GFI-1 UFK “Fialka” ultraviolet camera, SP spectrometer and HD (High Definition) camcorder, the experiment observes the Earth atmosphere and surface from window #9, with spectrometer measurements controlled from Laptop 3. “Relaxation”, in Physics, is the transition of an atom or molecule from a higher energy level to a lower one, emitting radiative energy in the process as equilibrium is achieved.]

The CDR also conducted the routine daily servicing of the SOZh system (Environment Control & Life Support System, ECLSS). [Regular daily SOZh maintenance consists, among else, of checking the ASU toilet facilities, replacement of the KTO & KBO solid waste containers and replacement of EDV-SV waste water and EDV-U urine containers.]

TJ Creamer worked an hour in the A/L, clearing out trash from the ULF3 EVAs and finishing up final tool configurations for the upcoming 19A spacewalks.

Working off his discretionary “time permitting” task list, Oleg Kotov had an another recording session with the SONY HVR-Z7U camcorder, shooting video of Lake Baikal. [Roskosmos TV studio is working on a feature on Lake Baikal and its importance as natural heritage, called ‘Planet Baikal’. The feature will be broadcast in Vesti channel’s weekly program Kosmonavtika. The Baikal Lake contains 20% of the world’s water reserves; it is a beautiful and a mysterious lake. The producers want to highlight the grandeur of this natural gem and raise awareness about its pollution problems. The metaphor used throughout the feature is one of a planet, an element of the Universe and a cosmonaut talking about Baikal while on orbit is thought to be a perfect choice to convey it. The feature item will be filmed and broadcast to Earth in real time later (April 6-9).]

Source:http://www.spaceref.com/news/viewsr.html?pid=33765

Nasa iss On-Orbit Status

March 26th, 2010

All ISS systems continue to function nominally, except those noted previously or below.

At wake-up, CDR Oleg Kotov performed the regular daily early-morning check of the aerosol filters at the Russian Elektron O2 generator which Maxim Suraev had installed on 10/19 in gaps between the BZh Liquid Unit and the oxygen outlet pipe (filter FA-K) plus hydrogen outlet pipe (filter FA-V). [FE-4 again inspected the filters before bedtime this morning, currently a daily requirement per plan, with photographs to be taken if the filter packing is discolored.]

CDR Kotov, FE-5 Noguchi & FE-6 Creamer joined up in the Soyuz 21S spacecraft (docked at the FGB Nadir port) for the standard 3-hrs Soyuz Emergency Descent Drill, regular procedure for each station crew. The exercise, which does not involve any command activation, uses computer simulation (Trenasher Spusk/”descent trainer”) on the RSK1 laptop with a descent hand controller (RUS) in manual mode to set up reentry conditions and switch between modes. [The onboard training (OBT) session, supported by TsUP instructor tagup, included a review of the pertinent RODF (Russian Operations Data Files), specifically the books on Soyuz Insertion & Descent Procedures, Emergency Descents, and Off-Nominal Situation Procedures such as manual undocking.]

After tearing down & removing the previously installed hardware of the GFI-1 “Relaksatsiya” (Relaxation) Earth Observation experiment at SM (Service Module) window #9 and closing the window’s interior protective cover for the duration of the Emergency Descent Drill, Kotov re-installed the gear for another experiment run, charging the battery for the SONY HVR-Z1J camcorder, then recording the planned GFI-1 activities, supported by ground specialist tagup. The gear was then closed out and removed. [Using the GFI-1 UFK “Fialka” ultraviolet camera, SP spectrometer and HD (High Definition) camcorder, the experiment observes the Earth atmosphere and surface from window #9, with spectrometer measurements controlled from Laptop 3. “Relaxation”, in Physics, is the transition of an atom or molecule from a higher energy level to a lower one, emitting radiative energy in the process as equilibrium is achieved.]

Timothy Creamer continued his major IFM (Inflight Maintenance) task on the CDRA (Carbon Dioxide Removal Assembly)’s bed #2 (202) started yesterday, supporting a sensor check by MCC-H ground commanding by removing the pin kit jumpers installed yesterday, then removing Bed #2 and installing new pin kit jumpers. [Objective of today’s activity was to avoid using LiOH (Lithium Hydroxide) canisters for CO2 absorption. Temperature sensor B of CDRA Bed 202 in the ARS (Atmosphere Revitalization Systems) Rack #2 located at LAB1D6 has shown some “out-of-family” temperature data. After yesterday’s task to bypass sensor B, only sensors A and C remained, but A showed a large bias and C is probably not connected, i.e., the bypass failed. Today’s task was to remove the jumpers, verify functionality of the sensors in their original configuration and then install new jumpers (22 gauge pin/socket) to connect Bed 202 sensors A & C while omitting temperature sensor B.]

In the COL (Columbus Orbital Laboratory), TJ worked on the BLB (Biolab), removing the spent silica gel dehumidifier bags from TCU1 (Temperature Control Unit 1) & TCU2 and replaced them with fresh ones.

In the MSL (Materials Science Laboratory), Creamer exchanged the used LGF SCA-5 (Low Gradient Furnace Sample Cartridge Assembly 5) with the next test sample (CETSOL #1). [The ESA/NASA MSRR-1 (Material Science Research Rack 1) provides a powerful multi-user MSL with diverse EMs (Experiment Modules) so that many material types, such as metals, alloys, polymers, semiconductors, ceramics, crystals, and glasses, can be studied in micro-G to discover new applications for existing materials and new or improved materials. MSRR experiments are coordinated by international teams that share different parts of the samples. There are 25 investigators on three research teams participating in the first of these investigations. CETSOL (Columnar-to-Equiaxed Transition in Solidification Processing) and MICAST (Microstructure Formation in Casting of Technical Alloys under Diffusive & Magnetically Controlled Convective Conditions) are two complementary material science projects, which carry out research into the formation of microstructures during the solidification of metallic alloys. The goal of MICAST is to study the formation of microstructures during casting of technical alloys. In space, buoyancy convection is eliminated and the dendritic solidification of the alloys can be quantitatively studied under purely diffusive conditions. The objective of CETSOL is then to study the transition from columnar growth to equiaxed growth that occurs when crystals start to nucleate in the melt and grow independently. Results of these experiments will help to optimize industrial casting processes.]

Soichi Noguchi had another 2h15m reserved for 19A cargo gathering & prepacking.

FE-6 conducted the weekly 10-min. CWC (Contingency Water Container) inventory as part of on-going WRM (Water Recovery & Management) assessment of onboard water supplies. Updated “cue cards” based on the crew’s water calldowns are sent up every other week. [The current card (23-0003) lists 95 CWCs (2,366.8 L total) for the five types of water now identified on board: 1. technical water (20 CWCs with 781.3 L, for Elektron electrolysis, incl. 87.5 L in 4 bags containing Wautersia bacteria, 134.2 L in 3 clean bags for contingency use, 559.6 L in 13 bags still requiring sample analysis, 2. potable water (9 CWCs with 366.7 L, of which 1 bag with 23.0 L contains Wautersia, 1 bag with 43.6 L requires sample analysis & 129.3 L in 3 bags are good for contingency use, 3. iodinated water (58 CWCs with 1089.1 L), 4. condensate water (4 bags with 105.4 L; 2 empty CWCs), and 5. waste/EMU dump and other (2 CWCs with 24.3 L). Wautersia bacteria are typical water-borne microorganisms that have been seen previously in ISS water sources. These isolates pose no threat to human health.]

In the SM, the Russian Commander did the routine daily servicing of the SOZh system (Environment Control & Life Support System, ECLSS). [Regular daily SOZh maintenance consists, among else, of checking the ASU toilet facilities, replacement of the KTO & KBO solid waste containers and replacement of EDV-SV waste water and EDV-U urine containers.]

Working off his discretionary “time permitting” task list, the CDR also performed the daily IMS (Inventory Management System) maintenance, updating/editing its standard “delta file” including stowage locations, for the regular weekly automated export/import to its three databases on the ground (Houston, Moscow, Baikonur).

At ~3:25am EDT, Oleg Kotov supported two PAO TV downlinks: (1) a message of congratulatory greetings for the 5th Anniversary of the Moscow Power Supply Company (“Thank you for reliable and uninterrupted power supply to Star City and Mission Control Center outside Moscow… Happy fifth anniversary to your company and its branches, one of them sharing the same Russian acronym MKS (Moscow Cabling Network) with our station…”); and (2) a Q/A exchange with schoolchildren currently participating in Russia’s social-science program “Step into the Future” at Bauman Moscow State Technological University (MGTU).

At ~3:41am, Soichi powered up the SM’s amateur radio equipment (Kenwood VHF transceiver with manual frequency selection, headset, & power supply) and at 3:46am conducted a ham radio session with students at Shiogama Daini Junior High School, Shiogama, Japan. [The school, WITH about 400 students and about 30 staff, was established as the second junior high school of Shiogama-city in 1947. Shiogama fish market is famous for a large quantity of bigeye tuna called "Higashimono". As Shiogama is a port city, there are a lot of people who engage in fishery and who utilize radio communication. Therefore there are many radio stations on the slightly elevated hill where people can look down at Matsushima-gulf.]

At ~12:00pm, FE-5 had his periodic PMC (Private Medical Conferences), via S- & Ku-band audio/video.

The crew completed their regular daily 2.5-hr. physical workout program on the ARED advanced resistive exerciser (FE-5, FE-6), T2/COLBERT advanced treadmill (CDR, FE-5, FE-6) and VELO ergometer bike with bungee cord load trainer (CDR).

ISS Reboost: Yesterday at 5:15am, Progress M-04/36P (at SM Aft port) performed a nominal single-burn reboost of the ISS with its 8 DPO (Rendezvous & Docking) thrusters, assisted by Progress M-03/35P (at DC1 Nadir port). The burn consumed 142 kg of propellant, about 3 kg of which was for attitude control before & after the burn. 36P mid-ring thrusters controlled ISS pitch & yaw and also provided the translation delta-V of 0.97 m/s (3.18 fps), while the radially docked 35P controlled ISS roll. Mean altitude gain was 1.7 km (0.8 nm). Purpose of the reboost was to set up phasing for the Soyuz 22S, 19A Shuttle launch, and Progress 37P launch.

WPA Update: On 3/22, the Water Processor Assembly, a sophisticated, complex system comprising the WWT (Waste Water Tank), various filters for particulates & contaminants, a gas/liquid separator, a catalytic reactor (to oxidize organics), an ion exchange bed (to remove reactor by-products), a heat exchanger, pumps, etc. to produce potable water from Lab waste water, went on Standby due to low temperatures in the preheater, probably due to cold water contacting the latter that the heaters could not compensate for. A subsequent attempt to bring the WPA’s catalytic reactor back up to temperature did not succeed. Also, it was noticed that the WWT was slowly losing contents (~3 lbm/day), indicating a possible leak somewhere. Valves within the WPA were closed to isolate the leak source overnight and the WPA was then fully deactivated and powered down. The plan is for the crew to go on a “hide-and-seek” tomorrow (3/26) in Node-3 to see where water may be leaking (rack umbilicals, internal to the rack?), which will require rotating the WRS-1 (Water Recovery System 1) and WRS-2 racks. While the WPA is down, the crew is using the Russian SRVK condensate processor for drinking water.

METOX Update: The METOX (Metal Oxide) regeneration initiated on 3/23 on the last remaining unregenerated METOX canister aboard appears to have completed successfully. This suggests that the two failed regenerations on 3/1 & 3/8 were likely due to those canisters being installed in the regeneration unit with the O-ring seals not fully seated (which allowed the heating gas to partially bypass the canisters and be ported into the regeneration unit enclosure, giving an erroneous temperature reading). The canister installation procedure will be updated accordingly.

CEO (Crew Earth Observation) photo targets uplinked for today were Yaounde, Cameroon (CEO staff has neither photography nor cloud-free satellite imagery of this target. However, rare combination of early morning timing and only hazy skies may permit views of this capital city of one and half million. As ISS tracked northeastward over the coast of Cameroon, the crew was to begin a nadir mapping strip to try and capture this city located inland within a rolling forested area of the country), Jerusalem, Israel (ISS had a mid-morning pass in fair weather over the Israeli capital located near the country’s center and less than 20 miles from the north end of the Dead Sea. This is a very low-contrast target. As ISS approached the Dead Sea from the SW, the crew was to look nadir for this city of three quarters of a million in the wooded hill country west of the northern Dead Sea), Baku, Azerbaijan (the capital city of Azerbaijan is located in the extreme eastern part of the country and situated on the south side of the Abseron Peninsula which juts into the southeastern Caspian Sea. ISS approach was from the SW in late morning with fair weather. As the station approached the coast of the Caspian Sea, the crew was to look nadir for this city of over 2 million), Megafans Central Algeria (this target area lies primarily to the left of track between two areas of darker rock northwest of the Hoggar highland area of southeastern Algeria. As ISS tracked northeastward over the northwestern Hoggar at mid-morning in clear weather, the crew was to try for context views of the megafan area left of track), and Tripoli, Libya (this capital city of 1.69 million has been occupied since its founding in the 7th century BC. It lies on a gentle bulge in the Libyan coastline. As the crew approached the Mediterranean coast from the SW at mid-morning in fair weather, they should have found this low-contrast target right on the coast at nadir

Source:-http://www.spaceref.com/news/viewsr.html?pid=33762

Get Adobe Flash playerPlugin by wpburn.com wordpress themes