DAYS IN SOLAR ROTATION INTERVAL ROT.­ NO. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 2289 Mar 29 30 1 5 10 15 20 24 Apr 2290 Apr 25 30 1 5 10 15 20 21 May 2291 May 22 25 30 1 5 10 15 17 Jun 2292 Jun 18 20 25 30 1 5 10 14 Jul 2293 Jul 15 PLANETARY MAGNETIC THREE­HOUR­RANGE INDICES Kp till 2001 Jul 15 = sudden commencement KEY 0 o + ­ 1 o + ­ 2 o + ­ 3 o + ­ 4 o + ­ 5 o + ­ 6 o + ­ 7 o + ­ 8 o + ­ 9 o

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• Format Documentation of *.wdc Files
• Geomagnetic Kp Index
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

... BDR FAX: (303) 497-6513 ------------------------------------------------------------------------------- SELECTED GEOMAGNETIC AND SOLAR ACTIVITY INDICES ------------------------------------------------------------------------------- WORLDWIDE INDICES -------------------------------------------------------------- The subscript p means planetary and designates a global magnetic activity in- dex ... 13-14 I2 Kp or PLANETARY 3-HOUR RANGE INDEX for 0000 - 0300 UT. ...

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• http://www.wdcb.ru/stp/data/geomagni.ind/kp_ap/kp_ap.fmt
• http://www.wdcb.ru/stp/data/geomagni.ind/kp_ap/11Kp_Ap_fmt.txt
• cat1aa

... 2015: . Detection of a Very Slow Magnetic Rotator HD 965 . Based on the measurements of the magnetic field of the chemically peculiar star HD 965, conducted in 2000-2015 with the SAO RAS 6-m telescope, we have found that this object is an ultraslow magnetic rotator with a rotation period of about 20 years. ... Detection of a Uniquely Bright Radio Flare in the X-Ray Binary Star with a Black Hole V404 Cygni (GS2032+336) . ... Detection of an OH Maser Flare in the Nebula W3 . ... Archive . ...

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We measured the spectrum of polarization for three proto-planetary nebulae (PPNs), IRAS 17411-2411, IRAS 08005-2356, and IRAS 04296+3429, and made model calculations with the dust-scattering Monte Carlo code DIRTY and the dust emission code 2Dust. ... Modeling the spectropolarimetry of IRAS 04296+3429 indicates a point-symmetric, multipolar morphology in the PPN phase. ... ADS Citation Query . citations = 11 . citations vs. year [year,citations] . ...

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Next: Astrometry Up: Calibrate data Previous: Calibrating amplitude errors Contents . There are three unwrapping algorithms available under C ALIBRATE V ISIBILITY T RIPLE . ... Rewrapping here shall mean the rotation of the complex visibility by a specified angle so that the entire range of phases fits into the interval degrees. ... If the phase is wrapping more rapidly, one should plot the (calibrated) triple phase, and fit a low order polynomial to a stretch which does not wrap (use FIT). ...

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The wave complex KEM-3 is designed to measure the parameters of electromagnetic waves in the VLF and ULF ranges. ... The electric antenna is a 1.6 m long dipole made up by two spherical carbon EDS detectors each with a preamplifier. ... The same detector is also used for the VLF device. ... 1. component Ex: 0.1 Hz - 400 kHz; 5*10E(-8)HzE(-1/2) (2 kHz). 2. component Bx: 1.0 kHz - 50 kHz; 10E(-5) nT*HzE(-1/2) (2 kHz). 3. components Bx,y,z: 1.0 Hz - 2 kHz; 3*10E(-5) nT*HzE(-1/2) (100 Hz). ...

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... GSAOI Home . ... Science . ... Despite vast increase in our understanding of the evolutionary nature of planetary nebulae (PNe) during the last three decades, a central question remains: where is the missing mass? Theoretical evolutionary tracks predict that all stars with masses in the range 1.4-8 M Sun should become PNe. ... Clearly, much of the mass of the planetary nebula shell must remain un-ionized, and much of it may be in molecular form. ... The Magellanic Cloud PNe are ideal for this. ...

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SET OF MAGNETIC AND ELECTRIC FIELD DETECTORS EXO-EM . ... 3 components measurements of both magnetic and electric fields; . ... wide frequency range (0 - 10000) Hz; . ... ECHO-EM is intended for measurement of a complete vector and three components of both electric and magnetic fields, and transfers the received data to the block of the processing of the information and also in telemetry. ... digital 0.1-20 Hz; . ... frequency band (0.01- 10000) Hz; . ... digital (500 - 1000) Hz; . ...

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... Programme . ... Abstract: Planetary nebulae constitute a unique source of light element abundances for individual stars in a distant stellar population. Multi-slit spectra of 50 planetary nebulae (PN) in NGC 5128 have been observed with the ESO VLT and FORS1 spectrometer. The planetary nebulae were observed in three fields covering a range of galactic radii from 2 to 19 kpc. The emission line spectra have been analysed for light element abundances (He, O, N, Ne, S, Ar). ...

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Proposal Identi cation No.: P1109 Date Received: 1997-Dec-16 17:03:27 Technical Page Proposal Type: Regular General Category: Pulsars Observation Category: Total Time Requested: 51 Hours Proposal Title: Probing the magnetic eld topology in millisecond pulsars ABSTRACT: At least three types of theoretical models have been developed to describe the magnetic eld topology in millisecond pulsar magnetospheres , ranging from distorted ... Maybe Part of the observing run. ...

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Determination of an Intermediate Perturbed Orbit from Range and Range Rate Measurements at Three Time Instances . ... Very Long Baseline Interferometry (VLBI), Small Solar System Body (SSSB), an intermediate perturbed orbit, a fourth-order tangency to the trajectory of perturbed motion, range measurements, range rate measurements, range observations, range rate observations, computing the preliminary orbit of a small celestial body, the degree of approximation of the real motion, the Keplerian orbit. ...

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... This document and the attached postscript figure document an analysis that I did to determine the optimum midpoint and required ranges for both the rotator and azimuth for the 2.5 M telescope. ... I simulate a series of drift scans on the sky for tracks that cover the northern survey area. These tracks cover the range in survey latitude of -60 to +60 degrees, spaced by 10 degrees. ... Along each track the azimuth, elevation, and position angle of the CCD is computed at 1 minute intervals. ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... H cores of four hot white dwarfs. Top to bottom: WD0446тИТ789 (magnetic according to Table 2, red line), WD 1620тИТ391, WD 2039тИТ202, WD 2007тИТ303 (all with longitudinal field consistent with zero), WD 1105тИТ048 (possibly magnetic, red line). ... Using FORS and UVES archive data, we have also revised numerous white dwarf field measurements previously published in the literature. ...

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Next: Observational Data Previous: Rotation Periods of PMS Stars . ... 1993,1995; Grankin 1993, 1994; Prosser 1993, 1994, 1995; Adams 1995; Choi & Herbst 1996) cover a wide range of stellar ages, but with exception of the ONC, the nTTs have been underrepresented. ... Because some nTTs may have very recently lost their disks, they could be stars undergoing rapid change in their rotational properties. ... 1996). In this dissertation, I will discuss the results of observations of nTTs in Orion. ...

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Feed cabin Nr. ... Fig. ... This allows to realize the sensitivity at frequency ranges 4.8, 11.2 and 30.0 GHz of 5, 7 and 12 mK by double beam switching mode and by the integration time of the output filter 1s. Input waveguide paths were very long and had big losses. ... The focal line of the feed cabin Nr. ... Data Acquisition and Control System . The Data acquisition system of the feed cabin Nr 2 is based on the new measurement ER-DAS system (Embedded Radiometric Data Acquisition System). ...

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• di_eks

... Ranger 9 was designed to achieve a lunar impact trajectory and to transmit high-resolution photographs of the lunar surface during the final minutes of flight. The spacecraft carried six television cameras, an optical earth sensor and high-gain antenna for optimum communications, and solar panels to provide power, as well as additional engineering equipment. ... The spacecraft encountered the lunar surface with an incoming asymptotic direction at an angle of -5.6 degrees from the lunar equator. ...

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... Moon Crashers . ... Seventeen minutes before impact it snapped this picture - the first image of the Moon ever taken by a U.S. spacecraft. ... Ozone Hole Reduced . ... Eta Carinae in X Rays . ... Eta Carinae is the one of the most luminous star systems in our Galaxy, radiating millions of times more power than our Sun. Eta Carinae is also one of the strangest star systems known, brightening and fading greatly since the early 1800s. Triton: Neptune's Largest Moon . ... Polaris: The North Star . ...

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... The table is used/accessed by: . CAL_getHKwindows() : Table with HK parameter validity data; data outside the given validity intervals may indicate degraded science quality and ought to be screened in the pipeline reduction by means of GTI filtering . ... 5-character short ID of parameter as found in the ODF HK data (e.g. F1123) . ... validity interval of the parameter in the form of a valid selectlib expression; '@' characters may be used instead of the parameter name; e.g. @ in [-91.0:-89.0] . ...

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... 2005 June 30 . Three Planets from Mt. Hamilton . Credit Copyright: R. Jay GaBany . Explanation: Venus, Mercury, and Saturn wandered close together in western evening skies last week. On Saturn day, June 25, astronomer R. Jay GaBany recorded this snapshot of their eye-catching planetary conjunction, from historic Lick Observatory on Mt. Hamilton , California, USA. ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ...

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... way these widgets work for the user. #include gtk/gtk.h GtkWidget *hscale, *vscale; void cb_pos_menu_select( GtkWidget * item , GtkPositionType pos ) { /* Set the value position on both scale widgets */ gtk_ scale _set_ value _pos (GTK_ SCALE (hscale), pos); gtk_ scale _set_ value _pos (GTK_ SCALE (vscale), pos); } void cb_update_menu_select( GtkWidget * item , GtkUpdateType policy ) { /* Set the update policy for both ...

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