Hard X-ray and gamma-ray spectrometer of high resolution and sensitivity on board the international space station (ISS)

2000 ◽  
Vol 25 (3-4) ◽  
pp. 901-904
Author(s):  
S.I. Svertilov ◽  
V.G. Stolpovskii ◽  
V.V. Bogomolov ◽  
M.I. Kudryavtsev ◽  
I.G. Mitrofanov ◽  
...  
2015 ◽  
Vol 56 (8) ◽  
pp. 1797-1804 ◽  
Author(s):  
Yu.D. Kotov ◽  
V.N. Yurov ◽  
Yu.A. Trofimov ◽  
E.E. Lupar ◽  
A.S. Glyanenko ◽  
...  

1998 ◽  
Vol 22 (7) ◽  
pp. 1057-1060
Author(s):  
M.I. Kudryavtsev ◽  
S.I. Svertilov ◽  
V.V. Bogomolov ◽  
A.V. Bogomolov

Author(s):  
Koji INAKA ◽  
Saori ICHIMIZU ◽  
Izumi YOSHIZAKI ◽  
Kiyohito KIHIRA ◽  
Elena G. LAVRENKO ◽  
...  

A series of space experiments aboard the International Space Station (ISS) associated with high-quality Protein Crystal Growth (PCG) in microgravity conditions can be considered as a unique and one of the best examples of fruitful collaboration between Japanese and Russian scientists and engineers in space, which includes also other ISS International Partners. X-ray diffraction is still the most powerful tool to determine the protein three dimensional structure necessary for Structure based drug design (SBDD). The major purpose of the experiment is to grow high quality protein crystals in microgravity for X-ray diffraction on Earth. Within one and a half decade, Japan and Russia have established an efficient process over PCG in space to support latest developments over drug design and structural biology. One of the keys for success of the experiment lies in how precisely pre-launch preparations are made. Japanese party provides flight equipment for crystallization and ensures the required environment to support the experiment aboard of the ISS’s Kibo module, and also mainly takes part of the experiment ground support such as protein sample characterization, purification, crystallization screening, and solution optimization for microgravity experiment. Russian party is responsible for integration of the flight items equipped with proteins and precipitants on board Russian transportation space vehicles (Soyuz or Progress), for delivery them at the ISS, transfer to Kibo module, and returning the experiments’ results back on Earth aboard Soyuz manned capsule. Due to close cooperation of the parties and solid organizational structure, samples can be launched at the ISS every half a year if the ground preparation goes smoothly. The samples are crystallized using counter diffusion method at 20 degree C for 1–2.5 months. After samples return, the crystals are carefully taken out from the capillary, and frozen for X-ray diffraction at SPring8 facility in Japan. Extensive support of researchers from both countries is also a part of this process. The paper analyses details of the PCG experiment scheme, unique and reliable technology of its execution, and contains examples of the application. Key words: International Space Station, Protein crystals, Microgravity, International collaboration.


2021 ◽  
Author(s):  
Andrey Mezentsev ◽  
Nikolai Østgaard ◽  
Torsten Neubert ◽  
Victor Reglero

<p>The Atmosphere-Space Interactions Monitor (ASIM) has been installed on board of the International Space Station in April 2018, successfully providing science data for 2.5 years. The Modular X- and Gamma-ray Sensor (MXGS) of ASIM is designed to detect Terrestrial Gamma-ray Flashes (TGFs) (short intense bursts of gamma-ray photons), produced during the initial breakdown phase of the +IC lightning discharges.</p><p> </p><p>In this contribution we report and summarize the results on the ASIM TFGs associated with high peak current lightning detections (detected by GLD and WWLLN networks). High peak current detections tend to be associated with short duration TGFs and do not exhibit a tendency to correlate with the fluence of the TGF.</p>


2014 ◽  
Vol 1 (1) ◽  
pp. 303-306
Author(s):  
Pere Blay ◽  
Lola Sabau-Graziati ◽  
Víctor Reglero ◽  
Paul H. Connell ◽  
Juana M. Rodrigo ◽  
...  

Atmosphere-Space Interactions Monitor (ASIM) mission is an ESA pay load which will be installed in the Columbus module of the International Space Station (ISS). ASIM is optimized to the observation and monitoring of luminescent phenomena in the upper atmosphere, the so called Transient Luminous Event (TLEs) and Terrestrial Gamma Ray Flashes(TGFs). Both TLEs and TGFs have been discovered recently (past two decades) and opened a new field of research in high energetic phenomena in the atmosphere. We will review the capabilities of ASIM and how it will help researchers to gain deeper knowledge of TGFs, TLEs, their inter-relationship and how they are linked to severe thunderstorms and the phenomena of lightning.


2002 ◽  
Author(s):  
Emi Miyata ◽  
Chikara Natsukari ◽  
Tomoyuki Kamazuka ◽  
Hirohiko Kouno ◽  
Hiroshi Tsunemi ◽  
...  

1997 ◽  
Author(s):  
William T. McdDonald ◽  
Johanna L. Lewis ◽  
Craig D. Smith ◽  
Lawrence J. DeLucas

1999 ◽  
Author(s):  
Lawrence DeLucas ◽  
William McDonald ◽  
Johanna Lewis ◽  
Craig Smith

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