... Transit times, hours . ... Date, time, UT . ... 111 . ... non-AR . ... 132 . ... 2000/02/12, 12 . ... 236 . ... 2001/03/20, 14 . ... 154 . ... 2004/01/22, 14 . ... Columns 2-6 - Information on the geospace disturbance, including the GMS peak date and time, minimum Dst and peak Ap values, FD magnitude, date and time of the disturbance onset (SC). ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... We study the magnetic field structure and evolution for 26 X-ray brightening events in coronal holes and quiet Sun regions, including bright points and jets. We found that all brightening events are associated with bipolar regions and caused by magnetic flux emergence followed by cancellation. ... Comparing coronal holes and the quiet Sun, we do not find differences in their corresponding magnetic field behavior. ...

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... are preliminary IAU-style names for ChaMP objects. Finalization of names awaits the final systematization of optical coordinates and source identification. ... The yellow regions highlight atmospheric telluric bands at ~6900A and ~7600A. The optical ID, X-ray ID, classification, and redshift are given at the top of each plot, and a series of lines are shown that are often found in sources of that given classification. ... HS limit? ... g' band magnitude; calibrated SExtractor Kron mag or limit . ...

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• Chandra Images for SNRJ 0540.1-6919
• Chandra Images for SNR J0535.7-6602
• *xflux, hxflux* - Calculation of X-ray Flux

... This file contains the information about IB_TAIL and IB_AUR (AURORAL) magnetic conjugations as a function of the Universal time. The predicted magnetic conjugations correspond to the less then 5 deg relative geocentric angular distance of the two satellites magnetic footprints. ... the difference between two satellites corrected geomagnetic local times (see as well column 11) . ... the difference between two satellites corrected geomagnetic latitude (see as well column 12) . ... AnD (deg) . ...

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• The summary plot of time distribution of the multisatellites magnetic
• Magnetic mapping
• The plot of the magnetic conjugation's time distribution

... The storm began quite unexpectedly. The strongest geomagnetic storm for the last seven months began on Earth almost precisely at the same time as the solar eclipse reached its maximal stage, the culmination of which occurred at GMT 02:35 (06:35 Moscow time). ... Oscillations of such amplitude in the magnetic field have not been observed since October, 11th of last year, which is more than seven months ago. ... We can only add that the magnetic storm lasted approximately 9 hours. ...

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• Magnetic storms online May 08, 2012
• Magnetic storms online August 31, 2014
• Magnetic storms online April 26, 2013

... It consists of a vertically arranged list of pushable buttons, each corresponding to one numeric, string, or boolean column found in the specified input table. Each button is labeled with the name of the column it represents. ... To the right of the button with the name of the column is a short framed label which specifies the types of the column: . ... 32-bit real . ... true/false To the right of this label are more GUI elements whose type depend on the type of the column. ... Integer columns . ...

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Radio data are displayed in the following format: . After the title with name of cluster under examination and with line about kind of data under one, e.g. Radio data [ optical data ] [ radio source identifications ] [ radio spectra (1.0 or 1.1) ] . ... The first line contains the number of radio sources associated with the cluster (these are just those sources with entries in sections 'Radio galaxy', 'Radio source' and 'Radio spectrum' below). ... Radio sources in cluster: 2 # . ...

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• Column label: MOONW
• Column label: OBSE
• Column label: MOONE

Optical Filters . The WFPC2 camera configuration and filter set require a substantial number of apertures for full utilization of its capabilities. ... An additional set of aperture names have been defined for use with the WFPC2 filters which require partial rotations. ... The pixel coordinates of these apertures will be reviewed on a regular basis to reflect changes in CCD and filter cosmetics. ... The aperture name is generally the same as the (rotated) filter name. ...

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• CSPICE Routines: INVORT_C
• NStars2A: Proper motions - the NLTT and 2MASS
• Python: module HTMLcolors

... Be/X-Ray Binaries and candidates in the Galaxy Up: Be/X-ray binaries and candidates Previous: Introduction . ... We separate galactic sources, systems in Large Magellanic Cloud (LMC) and in the Small Magellanic Cloud (SMC). ... In the first column we give sources names. ... Some comments and more detailed description of each object can be found in subsections "Comments to the tables" below (each subsection refers to galactic, LMC or SMC sources). ... Be/X-Ray Binaries and candidates in the SMC . ...

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• E-P transitions for different orbits
• Initial Distributions of Binary Parameters
• Massive X-ray Binaries

Program: PLOTSYM Purpose: Plot PGPLOT's marker- and Hershey symbols Category: PLOTTING, UTILITY File: plotsym.c Author: M.G.R. Vogelaar Keywords: GRDEVICE= Plot device: [LIST OF DEVICES] Destination of plot, Screen or Hardcopy. OPTION= 1=Plot markers, 2=Plot Hershey symbols: [1] 1: Plot one page with rows x columns graph markers starting with marker index -1. ... Boxes with undefined Hershey symbols are not displayed, so the symbol numbers are not consecutive. ... PGWIDTH= Give line width 1.. ...

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• http://www.atnf.csiro.au/research/pulsar/psrtime/tempo2/versionChanges.html
• http://www.atnf.csiro.au/computing/software/gipsy/tsk/fit.dc1
• casacore: casa::RowCopier Class Reference

Taking into account the result by Watanabe P=2.5 days in outburst, I reconstruct old set of photographic observations being partly lost, and add some new observations. ... The periodogram calculated with the method by Lafler and Kinman is shown. ... The last periodogram indicates peaks corresponding following possible periods with the double-wave light curve: 0.4236, 0.4650, 0.5379, 0.6064, 0.7365, 0.871, 1.168, 1.5437, 2.8173, and 6.89 days. ...

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• http://mavr.sao.ru/hq/lizm/conferences/pdf/2003/2003_p216.pdf

The .out files contain the data displayed in plots of the wide spectral scans of High-CAL and the respective bets-fits obtained. Each of the 14 pipelines has a separate file. What to expect inside this file ? ... These files are made available for interested people to download. ... Note: Since the measurements for the beam0-pol_1, beam 5 (both pol.s) were missed from the set on tJD:53228 (due to the pre-amp and WAPP problems respectively), the corresponding fits & .out files missing. ...

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