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7101. List of the Experiments, PI and Key Scientists
. Last update 29 November 1996 by Pavel Eiges
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Ссылки http://www.iki.rssi.ru/tail/list.html -- 1.8 Кб -- 27.12.1996
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7102. POLRAD Results Page
An example of the AKR (Auroral Kilometric Radiation) recorded by the POLRAD radio-spectro-polarimeter. The 3 perpendicular components of the electric field are presented in the range from 4 kHz to 1 MHz , while crossing the morning sector of the auroral region (3.00 - 5.40 MLT) at the altitudes from 14441 to 18392 km. The lower limit of the AKR was at 150 kHz, while the maximum power was received at a typical range from 200 to 400 kHz. ...
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Ссылки http://www.iki.rssi.ru/auroral/polrad.htm -- 2.5 Кб -- 28.11.1996
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7103. DOK-2 Results Page
The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...
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Ссылки http://www.iki.rssi.ru/auroral/dok2.htm -- 9.9 Кб -- 28.11.1996
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7104. KM-7 Results Page
The primary purpose of KM-7 is to measure the temperature of cold electrons Te in Plasmasphere. ... The spacecraft potential can be evaluated from these measurements. ... MLT . ... Fig.1 . KM-7 measurements in MRK mode during the whole orbit 124 , 27.IX.96. ... Preliminary results . In period considered SC passed the plasmasphere at low and middle latitudes near L < 4 at heights = 8000-10000 km. At L > 4-5 and heights > 8000-10000 km SC was in auroral zone. ...
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Ссылки http://www.iki.rssi.ru/auroral/km7.htm -- 3.9 Кб -- 26.11.1996
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7105. BNS Results Page
. Fig.1 . Compressed magnetic field data from IMAP-3 through BNS-M . In the middle - the perigee crossing. Fig.2 . Solar detectors data. Area with zero signal corresponds to the part of the orbit where SC was in shade. Fig.3 . Expanded part of Fig.2 . From this data one could get an idea about orientation quality: the curve must be a sine wave if orientation is good. Fig.1 . Fig.2 . Fig.3 .
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Ссылки http://www.iki.rssi.ru/auroral/bns.htm -- 2.3 Кб -- 26.11.1996
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7106. IESP-2M Results Page
. An example of ULF electromagnetic fields detection by the IESP-2M instrument. The figure presented is the dynamic spectrogram. E and B components are measured in satellite coordinates. Observations were made in the auroral region. Electromagnetic turbulence, which was observed mostly in electric components, is typical for this phenomenon. Fig.1 .
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Ссылки http://www.iki.rssi.ru/auroral/iesp2m.htm -- 2.0 Кб -- 26.11.1996
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7107. PROMICS-3 Results Page
. Fig.1 . Auroral oval crossing in postmidnight-morning sector. In the middle - plasma sheet protons, at the sides - ring current protons. The five panels - count rates at different directions to the satellite rotation axis. Fig.2 . Auroral electrons above the nightside oval on the left, and above the dayside oval - on the right. Fig.1 . Fig.2 .
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Ссылки http://www.iki.rssi.ru/auroral/promics3.htm -- 2.1 Кб -- 26.11.1996
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7108. Marina Shevchenko Home Page
. Space Research Institute Webmaster . Department Number . 81 . Postal Address . 117810 Space Research Institute . Russian Academy of Sciences . Profsoyuznaya St. 84/32 . Moscow, Russia . Telephone Number . +7(095) 333-1488 . Fax . +7(095) 333-2089 . email . mshevche@arc.iki.rssi.ru .
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Ссылки http://www.iki.rssi.ru/people/mshevche.html -- 1.7 Кб -- 16.11.1996
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7109. TNP Host
The primary copy of The Nine Planets is located at SEDS at the Lunar and Planetary Laboratory , University of Arizona in Tucson, Arizona, USA. There are many other interesting space-related items at this site. The Nine Planets is also mirrored at several other sites around the world. Please use the one nearest to you... Introduction ... Overview ... Sun ... Bill Arnett ; last updated: 1995 June 11
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Ссылки http://www.iki.rssi.ru/nineplanets/host.html -- 2.0 Кб -- 08.11.1996
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7110. ENERGETIC PARTICLE EXPERIMENT DOK-2
ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...
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Ссылки http://www.iki.rssi.ru/interball/dok.html -- 12.3 Кб -- 30.10.1996
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7111. CONPAS workshop: Sessions Archive
Click in the sell of the table to see an agenda of the session | 1994 | 1995 | 1996 | __________|______|______|______| | | | | January | | * | * | Febuary | | * | * | March | | * | * | April | | * | * | May | | * | * | June | | * | * | July | | * | | August | | | | September | | * | | October | | * | Next | Nobember | * | * | | December | * | | |
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Ссылки http://www.iki.rssi.ru/CONPAS/Archive.html -- 2.1 Кб -- 23.10.1996
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7112. Next session; Oct 29, 1996 CONPAS workshop
Next session of a regularly functioning workshop "Computer Networks: Problems Solutions" will be held on Tuesday, Oct 29, 1996 at 11.00 a.m. The session will take place in Space Research Institute, Russian Academy of Sciences. ... Send your requests to Andrew Ananjev , secretary of the Workshop, by Email: andy@iki.rssi.ru or by phone: (095) 333-24-02 . Following information essential: Your Full Name (including fathers name), and Organization. ... Return to CONPAS homepage . ...
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Ссылки http://www.iki.rssi.ru/CONPAS/Oct96.html -- 2.7 Кб -- 23.10.1996
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7113. Next session; June,18 1996 CONPAS workshop
Next session of a regularly functioning workshop "Computer Networks: Problems Solutions" is expected to be held on Tuesday, June 18, 1996 . Nikolay Isakiv nisa@novell.msk.ru . " Recommended Solutions for Educational Organizations from NOVELL " . Agenda of the Next Session . Agenda of the Previous Session . Return to CONPAS homepage .
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Ссылки http://www.iki.rssi.ru/CONPAS/Jun96.html -- 2.0 Кб -- 23.10.1996
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7114. dok-2 Fig.3
Time averaged spectra for 1e (upper panels) and 1p (bottom panels) telescopes for two events in the magnetotail plasma sheet 27-28.11.1995.Exponential and power law approximations to experimental spectra are given by smooth curves with parameters indicated right of the spectra.
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Ссылки http://www.iki.rssi.ru/interball/fig3.html -- 1.4 Кб -- 22.10.1996
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7115. dok-2 Fig.4
Examples of energetic spectra shapes during non-stationary particle fluxes.
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Ссылки http://www.iki.rssi.ru/interball/fig4.html -- 1.2 Кб -- 22.10.1996
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7116. Examples of the raw magnetic field information, obtained with the MIF-M
... Tpram - time of the PRAM instrument (aquisition computer) . ... Bx - DC magnetic field with a fixed amplitude calibration; X component . ... The color lines present FFT from the AC magnetic field (Waveform); Bwx, Bwy, Bwz - from the bottom. ...
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Ссылки http://www.iki.rssi.ru/interball/aspi/pramv.html -- 2.9 Кб -- 17.10.1996
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7117. Attitude determination example
... The example demontsrates a way how to use the coefficients arrays and the Software . Let us suppose that we have a direction in the S/C frame, determined by the angles u1, u2, where: u1 - angle between vector and X axis (polar angle) u2 - angle on the YZ plane from Y axis (anticlockwise); . ... We use the file 950909t1 (the beginning data 9.09.06), which line 2 interval beginning : date 10.10.95 , time 1.926 thousands of sec, the interval duration is 4.583 thousand of sec. ...
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Ссылки http://www.iki.rssi.ru/interball/attitude/aexample.html -- 2.5 Кб -- 19.09.1996
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7118. Fortran subroutine attid1
... subroutine attid1 (ts,u1,u2, dir ) common /z/ z(2) common /c/ x(12) dimension s(3),e(3),p2(3), dir (3), dra (3),pa(3,3) ux= atan (1.)/45.*u1 uy= atan (1.)/45.*u2 dra (1)= cos (ux) dra (2)= sin (ux)* cos (uy) dra (3)= sin (ux)* sin (uy) alf=x(1)+x(2)* sin (x(11)*ts)+x(3)* cos (x(11)*ts)+x(4)* sin (x(12)*ts)+ *x(5)* cos (x(12)*ts) bet=x(6)+x(7)* sin (x(11)*ts)+x(8)* cos (x(11)*ts)+x(9)* ...
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Ссылки http://www.iki.rssi.ru/interball/attitude/attid1.html -- 3.1 Кб -- 19.09.1996
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7119. http://www.iki.rssi.ru/da/apex.srt
apex / 0124 apex / 0242 apex / 0312 apex / 0348 apex / 0359 apex / 0359_2 apex / 0430 apex / 0442 apex / 0454 apex /0465 apex /0477 apex /0477a apex /0489 apex /0501 apex /0513 apex /0524 apex /0572 apex /0583 apex /0595 apex /0618 apex /0642 apex /0690 apex /0784 apex /0807 apex /0820 ...
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Ссылки http://www.iki.rssi.ru/da/apex.srt -- 2.2 Кб -- 26.08.1996
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7120. http://www.iki.rssi.ru/da/activ.srt
activ / 00021 activ / 00022 activ / 00038 activ / 00043 activ / 00044 activ / 00067 activ / 00069 activ / 00069.a activ / 00080 activ /00100 activ /00105 activ /00117 activ /00137 activ /00150 activ /00167 activ /00173 activ /00178 activ /00186 activ /00192 activ /00204 activ /00229 activ /00235 activ /00241 ...
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Ссылки http://www.iki.rssi.ru/da/activ.srt -- 7.8 Кб -- 26.08.1996
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