... Future seminars . P a s t seminars . ... Almost monoenergetic ions – new source of information on the dynamics of space plasma current sheets " . ... Lutsenko (IKI) . ... Such spectra shapes were observed tens of years in multiple experiments on spacecrafts and followed from current theoretical models. ... This hypothesis explained all main observed AMI features. ... The AMI discovery gives a new support of H. Alfv n ideas on a great role of electric currents in a space plasma. ...

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Interferometric studies of the mass-loss process from cool evolved stars . ... Observing with ESO Telescopes . ... Cool evolved stars of different inital masses and thus luminosities loose considerable amounts of processed material and dust into the interstellar medium. ... However, the detailed mass-loss process is surprisingly little understood for most of these sources. ... Return to list of thesis topics . ...

The "ring of fire" seen by satellite cameras around the polar caps (picture below) is probably created by electrons leaking from the tail's plasma sheet, whose magnetic field lines form a somewhat imperfect trap. ... One possible explanation involves the close association between auroral arcs and electric currents which flow along field lines between the ionosphere and distant space ( Birkeland currents ). ... That produces an extra resistance to the flow of current. ...

... The process of proposing for Hubble Space Telescope observing time has been revised, to make it simpler for proposers. We describe the simple, flexible, and robust prototype system created to handle proposal submission. ... Proposing for Hubble Space Telescope ( HST ) observing time proceeds in two phases: the scientific merits of the proposal are considered in Phase I; only accepted proposals enter Phase II, where the observations are described in complete detail. ...

... Psrcat . Data archive . ... PSRCORR receives data from PKCCC1 , and displays, processes and archives them. ... Click on Setup and select WBA and old tape or new tape as appropriate. ... At the end of each observation the raw data files are written to the archive tape and the file details recorded in the tape log which is located in /psr1/runtime/psrcorr/db/tape.log . ... This allows you to select an archive tape and the file(s) to be archived (from PKCCC1 _1) and to write these files to the tape. ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

Next: Conclusions Up: Adaptive Least Squares Image Previous: Processing of Simulated . Fig. 6 shows an image of Saturn which was recorded with the Wide Field / Planetary Camera. It is stored in the file SATURN.FITS. The measured point spread function from the data file SATURN_PSF.FITS is also displayed. Fig. 7 shows the result of restoration. The restored image appears much clearer, with higher contrast than the measured data. ... Thu Jun 2 15:47:14 EDT 1994 ...

Irregular phenomena in the Earth Pole oscillation process and temporal variations of geopotential Valery Bondarenko, Vadim Perepelkin s The observed irregular phenomena in the Earth Pole oscillation process are very variety. ... These phenomena indicated in the IERS data are the "abnormal" fluctuation of the Earth Pole coordinates which owing to changing of the geodynamical parameters gives negative result in interpolation and forecast of the first approximation mathematical model. ... Fig. ...

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

... Mokhovaya st., 11, Moscow, 103907, Russia. ... Proceedings of International Seminar on Nonlinear Circuits and Systems, Moscow, Russia, June 16-18, 1992 , vol.1, pp. ... The principles of information processing (storing information, associative memory, image recognition) in nonlinear systems with dynamic chaos are studied. The use of complex dynamic regimes in solving certain information problems is shown advantageous with respect to the methods based on simple dynamics. ...

... Astronomical image processing applies a large variety of numerical methods to extract scientific results from observed data. The standard computational techniques used in this process are discussed with special emphasis on the problems and advantages associated with them when applied to astronomical data. ... In Section the transformation of raw observed data into intensity calibrated values is discussed while general image processing techniques are reviewed in Section . ... Basic Concepts . ...

... Kashyap, V., Drake, J., Smith, R., & Wargelin, B., 2014, 15 Years of Science with Chandra Symposium, Spectrum Ultimum Capellae: XV Years of Chandra Observations of Capella . ... Kashyap, V.L., Connors, A., Drake, J., Lee, T., Posson-Brown, J., Saar, S., Scargle, J., van Dyk, D., & Wong, R., 2014, AAS/HEAD 14, 119.05 TANAGRA: Timing Analysis of Grating Data . ... Audard, M., G del, M., Drake, J.J., & Kashyap, V.L., 2000, ApJ, 541, 396 . Audard, M., G del, M., & Guinan, E.F., 1999, ApJ, 513, L53 . ...

Since the first stars and then galaxies formed the Universe has been an immense factory converting neutral gas into stellar material. ... In this seminar I will discuss recent results from the Galaxy And Mass Assembly (GAMA) survey, probing the assembly of stellar mass though both in-situ star formation (as traced by multiple SFR indicators) and interactions (both mergers and interaction induced star-formation) - in galaxies spanning ~4 decades in stellar mass. ...

... 2) SIRTF Science Center, Caltech, MS 100-22, Pasadena, CA 91125 . ... In the near and mid-IR, its morphology is similar to that expected for a jet driven outflow, where the leading bow shocks entrain and accelerate the surrounding molecular gas. ... The H$_2$, H$_2$O and CO molecular emission could arise further `downstream' at the bow shock wings where the shocks (v = $8 - 35$ \kms) are oblique and more likely to be C-type. ... The millimetric continuum emission shows two sources. ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... The interface between the lower solar atmosphere where energy is generated by subsurface convection and the corona comprises the chromosphere, which is dominated by jet-like, dynamic structures, called mottles when found in quiet regions, fibrils when found in active regions and spicules when observed at the solar limb. ... In addition, how they affect the coronal heating and solar wind need to be further explored. ...

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

... Acceleration of particles in the vicinity of a massive black hole We propose a two-step mechanism for charged particle acceleration in the magnetosphere of a massive black hole surrounded by an accretion disk. Particles first gain energy by stochastic process during the accretion phase. It is shown that effective proton acceleration up to energies eV is possible in the turbulent magnetized accretion disk. ...

... B.V. Somov . head of the department . ... room 80 . ... senior research felow . ... research felow . ... research fellow . ... Our department performes the following most perspective studies: . Special analytical and numerical experimental investigations of the solar plasma involved in the magnetic reconnection process at the Sun. ... Head of the seminar: Prof. B.V. Somov. ... 27 September 2013 The Solar Physics Department was visited by journalists of the leading Russian TV channel "Vesti-1". ...

... в конференц-зале ГАИШ в 14 00 . ... Секретарь семинара М.К. Абубекеров . ... Липунов В.М. (ГАИШ МГУ) . ... Бескин В.С. (ФИАН РАН) . сопредседатель . ... Митрофанов И.Г. (ИКИ РАН) . ... Постнов К.А. (ГАИШ МГУ) . ... Курт В.Г. (АКЦ ФИАН) . ... Прохоров М.Е. (ГАИШ МГУ) . ... Имеется огромная потребность в обмене идеями и информацией сильно разделившихся в последние годы астрономических центров - ГАИШ, ФИАН (теор отдел), ИТЭФ, АКЦ ФИАН, Институт Астрономии, ИКИ, ИПМ, Институт Физпроблем, ИЯИ .. ...

... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...