. The page is under construction. Our table shows a classification of various light scattering methods, applicability to different scatterers and to their ensembles as well as the anzatz sources and recent reviews. In comments we briefly discuss different classifications, features, relationships, available codes, comparison works and recent reviews of the light scattering methods. To the top . Created by V.I. Last modified: 10/04/03, V.I.

do mod_pw (must be run from LRP account) . ... SU 0nnnn01 PC: xxxx cycle: 5 orb: 6 st.stat: scheduling in SPSS: Y cw_stat: S orient: Y type: GO/WFI pws.stat: planned S: Y proc_err: N lrp _state: ready LRP : 97073A ----------------------------------------------------------------------- QSP order_num: ( NONE ) week_id: ( NONE ) exe_time: ( NONE ) USC 1996.001:00:00:00 1997.054:00:00:00 M:c C:17-Feb-1997 N:FGS23GS Comment : Visit was unschedulable or had no FGS23 GSs when ...

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... These energies are from LS coupling and so there is no fine structure splitting. % produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % Peter Young, Feb 2000 . contains wavelengths, gf and A values for each transition. ...

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Low cost beginner eyepieces. Send SASE for price list. ... Listed Since October 26, 2004 . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... 30 Mar 2004 Corrected : jo1031.html, jo1031.txt, fjupoout.html ----------- 22 Mar 2004 jo1033.txt, so1012.txt Modified : (Column 'Old Ident' erased) fjupoout.html , fsapoout.html , fjupogal.html, fjupoinn.html, fmapomai.html, fnepomai.html, fnepoout.html , fsapoinn.html, fsapomai.html, furpoinn.html, furpomai.html , furpoout.html ----------- 20 Feb 2004 jo1032.txt Modified : fjupoout.html ----------- 15 Jan ... Line with jo0024 in the file fjupoout.html was corrected. ...

... W401, W402 ... codes are for AO4 experiments. ... EXPNO SOURCE FRQ Corr DOY DY: DATE UT RANGE #TEL TELESCOPES VS01s J2225-04 C Pent 337 Sa:Dec-02 07:00 - 13:00 7 HH UD SH MP CD HO VS09p J2320+05 C Pent 343 Fr:Dec-08 10:00 - 18:00 8 HH NT TR CD UD SH MP W001e J2358-10 C Pent 345 Su:Dec-10 09:00 - 14:00 8 HH NT AT TR HO UD MP VS06k W022a9 J1230+12 L Socr 354 Tu:Dec-19 08:00 - 17:00 15 VLBA GO EB UD SH W040a7 J1230+12 C Socr 355 We:Dec-20 08:00 - 13:00 13 AR VLBA Y W023b4 J1219+05 L ...

. Comment on J0042+2320 . 8.4 GHz VLBI image from the USNO database shows a N-NE extension of 4 mas which is not visible in our image due to the lack of resolution in that direction. VLBApls home page . Last modified: 16 Oct 2000

... The accuracy of calculation of both INTERBALL spacecraft (SC) motion has been estimated at the IKI. ... The 30 days measuring intervals were used during the Tail probe (TP) orbital data treatment, and 15 days intervals - during the Auroral probe (AP) orbit determination. ... http://www.iki.rssi.ru/vprokhor/indap.htm for the Auroral probe; . http://www.iki.rssi.ru/vprokhor/indtp.htm for the Tail probe . ... http://www.iki.rssi.ru/vprokhor/ssc.htm , or http://www.iki.rssi.ru/vprokhor/amisan.htm . ...

Next: The Quasi--Newton Method. Up: Outline of the Previous: The Newton--Raphson Method. ... At each iteration, one computes . ... Neglecting the second derivatives matrix , we obtain the ``normal equations'' and the Gauss--Newton direction . This so--called Gauss--Newton method is intended for problems where is small. ... The algorithm implemented here is a modification of that Gauss--Newton method, that allows convergence even for rank deficient Jacobians or for large residuals. ...

Trace: benchmark . start : benchmark . ... SAI VO Projects . ... AstroSearch . AstroDB . AstroKeywords . ... Help on Wiki search . ... benchmark.txt Last modified: 2011/12/27 17:19 by karpov Back to top . SAI VO | Astronet | SAI MSU | ...

... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...

... SPICE System Documentation . Comprehensive set of SPICE System documentation including tutorials, subroutines and data formats descriptions, etc. Other related home pages