... The variability of the spectrum of the optical component of the IR-source IRAS01005+7910 was discovered for the first time in the BTA spectra [1]. ... The spectral features include absorptions that form in near-photospheric layers, narrow envelope emissions, and emission-absorption profiles that form in photosphere-to-envelope transition layers (the wind). ... Discovery of spectral variation in the optical counterpart of IRAS01005+7910. ... Dashed line - envelope curve of all the SiII 5979 profiles ...

... The plasma region above the ionosphere on such closed magnetic field lines is called the plasmasphere. ... In the first approximation, the plasmasphere lies just inside the ring current and the plasma sheet field lines. ... In addition, plasmasphere is asymmetric, having a clear dusk side bulge (Carpenter, 1970; Chappell et al., 1970; see also Carpenter et al., 1993) that swings westward during high geomagnetic activity (Carpenter, 1970). ... Res., ... 75 , 3837-3847, 1970 . ... 75 , 3848-3861, 1970...

... Centrifuge . ... Technical description centrifuge TSF-7 . ... If during rotation the operator feels badly, the hand will release, and the centrifuge will stop. ... Tests for cosmonauts: . ... Services / Centrifuge: General description Technical description Photo gallery Price . Info: Industry news On-line Data Company ATLAS news Events We in press Contact . Copyright 2000-2016 ATLAS Aerospace . ...

... The air just sit there and doesn't get stirred. ... Normally, the air is hottest near the ground and gets cooler as you go up. ... If it weren't for the temperature profile, convection wouldn't occur: Because the temperature decreases with altitude, cold air sits on top of hot air, allowing convection. ... The air above the ground is hot, the air above the water is cold. ... The land cools down faster than the sea, so the air above the ground is colder than the air above the water. ...

COPRATES CHASMA NORTH WALL INTERIOR LAYERED DEPOSIT: LAYER MEASUREMENTS AND COMPARISON WITH JUVENTAE CHASMA ILDS USING MARS EXPRESS HIGH RESOLUTION STEREO CAMERA (HRSC) DERIVED TOPOGRAPHY Michael, G.1, E. Hauber1, K. Gwinner1, R. Stesky2 ... Planets, Freie Universitaet, Berlin, Germany 5ESTEC, ESA, Noordwijk, The Netherlands Introduction: The interior layered deposit ( ILD ) in the north wall of Coprates ... The lesser section of the ILD is confined by a ridge of the chasma wall. ...

Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...

... Line radiative transfer in C 18 O, HCO + , and CS lines is considered in a spherically symmetric chemo-dynamical model of a starless core, evolution of which is driven by the ambipolar diffusion. Theoretical line profiles are compared to observational data on the well-known L1544 core, which is one of possible candidates for collapsing protostellar clouds. ... Comparison between modelled and observed spectra suggests that L1544 has flattened structure and is observed at some inclination. ...

... USE_LOCALE = 1 + # If you plan to use Kerberos for authentication.. 716,4 +721,9 @@ CFLAGS+= -DNO_ASSERT_CHECKING endif + + ifdef USE_LOCALE + CFLAGS+= -DUSE_LOCALE + endif + ifdef PROFILE --- src /backend/main/main.c.ORG Fri Nov 15 02:00:31 1996 +++ src /backend/main/main.c Thu Apr 3 18:00:38 1997 @@ -15,4 +15,7 @@ # include string.h # include unistd.h +# ifdef USE_LOCALE + # include locale.h +# endif # include postgres.h # ...

... The software enables to browse HITRAN-86 or 96 databases. It enables input first 7 atmospheric gases. ... calculate atmospheric transmittance on any pressure level, . calculate instrument transmission functions through the atmosphere, . ... The software is supplied by standard atmospheric profiles, extracted from FASCODE_3.0 FORTRAN codes (dowloaded from PL/GP), and by instrument response function for IR channels of NOAA 14 satellite (both AVHRR and HIRS, downloaded from NOAA/NESDIS). ...

... Name (for family membership, include all family member names) Address City, State, Zip Code Home Phone Email Address Other Phone Alternate Email Occupation (if retired, list previous occupation; if student, list major) Employer or School My Employer will match my donation Membership List ­ Each year we publish our Membership List with name, city, email and home phone number and distribute this list to all members. ... Student Memberships are for FULL TIME students of any age. ...

TiTanTM ION PUMPS TiTanTM ION PUMPS TiTanTM ION PUMPS Ion pumps are used in a wide variet y of high and ultra - high vacuum (UHV) environments. ... Gamma Vacuum maintains stock of the most common confi gurations for same - day deliver y. These pumps have the added advantage that they can be mounted in any o r i e n t a t i o n w i t h o u t a d d i t i o n a l s u p p o r t. LOW PROFILE ION PUMPS (100L - 1200L X) Low Profile ion pumps are under 12 in. (300 mm) high for standard confi gurations. ...

... Authors: F. Camilo et al. astro-ph/0610769 Трехмерное распределение межзвездной среды в Галактике: II. ... Authors: J. Bouwman et al. обзор astro-ph/0610423 Атомные данные для рентгеновской астрофизики (Atomic Data for X-ray Astrophysics) . ... astro-ph/0610840 Магнитовращательный коллапс массивных звездных ядер в нейтронные звезды: моделирование с учетом эффектов ОТО (Magnetorotational collapse of massive stellar cores to neutron stars: Simulations in full general relativity) . ... Authors: Piet...

We present a catalogue of galaxies for which spatially resolved data on their internal kinematics have been published; there is no apriori restriction regarding their morphological type. The catalogue lists the references to the articles where the data are published, as well as a coded description of these data: observed emission (E) or absorption (A) data, optical (O) or radio (R) data, velocity (V) or velocity dispersion (D), radial profile (1) or 2D field (2). ...