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1381. http://www.izmiran.rssi.ru/~obridko/papers/47.pdf
... Polarization spectrograms were obtained by two spectrographs (prism and echelle types) during the solar eclipse in Mexico on 7 March, 1970 near the region of the second contact at the heights 0.06 to 0.12 R| above the limb. ... A negative reproduction of the coronal spectra. (a) Spectrum obtained by two-prism spectrograph; exposure time 20 see; (b) Two parts of the first 7 sec spectrum near the green and red lines obtained by echelle spectrograph. ... ET height 1.08 R o was equal to 30_ 5%. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/47.pdf -- 694.9 Êá -- 22.03.2011
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1382. http://www.izmiran.rssi.ru/~obridko/papers/190.pdf
STRUCTURE AND CYCLIC VARIATIONS OF OPEN MAGNETIC FIELDS IN THE SUN V. N. OBRIDKO and B. D. SHELTING IZMIRAN, 142092, Troitsk, Moscow Region, Russia (Received 28 October 1997; accepted 2 March 1999) Abstract. The structure and variations of open field regions (OFRs) are analyzed against the solar cycle for the time interval of 1970 ´ 1996. ... This supports the concept of a single complex ´ `large-scale magnetic field ´ active region ´ coronal hole'. ... Butterfly' diagram of the open field. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/190.pdf -- 355.8 Êá -- 22.03.2011
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1383. http://www.izmiran.rssi.ru/~obridko/papers/31.pdf
ON THE ENERGY DISSIPATION RELEASE IN THE BY MAGNETIC FIELD SOLAR ATMOSPHERE M. KOPECKY and V. OBRIDKO* Astronomical Institute of the Czechoslovak Academy of Sciences, Ond(ejov (Received 18 April, 1968) Abstract. ... 1) The calculations of the conductivity for the case of fully ionized gas gave very great values for all layers in the solar atmosphere. ... 2) What is the value of the energy released by magnetic-field dissipation, and how large is the heating of atmospheric layers by this process? ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/31.pdf -- 245.5 Êá -- 22.03.2011
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1384. http://www.izmiran.rssi.ru/~obridko/papers/171.pdf
FOURIER PARAMETERS AND MOMENTS POLARIZATION PROFILES OF MAGNETICALLY LINES. ... A new method is proposed to determine all components of the solar magnetic fields using the cumulants of the profile of a magnetic sensitive line. The method is based on polarization measurements in a number of points of the line profile and subsequent calculation of the amplitudes and phases of its two first Fourier-harmonics. ... Use these to find two or three first cumulants of the line profile. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/171.pdf -- 350.4 Êá -- 22.03.2011
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1385. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110321.txt
ÎÁÇÎÐ ÑÎÑÒÎßÍÈß ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ, ÃÅÎÝÔÔÅÊÒÈÂÍÛÕ ßÂËÅÍÈÉ È ÈÕ ÂÎÇÄÅÉÑÒÂÈÉ ÍÀ ÎÊÎËÎÇÅÌÍÎÅ ÊÎÑÌÈ×ÅÑÊÎÅ ÏÐÎÑÒÐÀÍÑÒÂÎ ÍÀ ÏÅÐÈÎÄ 14 - 20.03.2011 ã. È ÏÐÎÃÍÎÇ ÍÀ 21 - 28.03.2011 ã. ÊÝÐÐÈÍÃÒÎÍÎÂÑÊÈÅ ÎÁÎÐÎÒÛ 2107, 2108 (16,73.02; 16,06.03.2011) ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÀß ÀÊÒÈÂÍÎÑÒÜ ÑÎËÍÖÀ ÏÐÎØÅÄØÅÃÎ ÏÅÐÈÎÄÀ ÇÍÀ×ÈÒÅËÜ- ÍÎ ÑÍÈÇÈËÀÑÜ, È Â ÊÎÍÖÅ ÏÅÐÈÎÄÀ ÁÛËÀ ÍÀ ÍÈÇÊÎÌ ÓÐÎÂÍÅ. ... ÍÀÈÁÎËÅÅ ÂÅÐÎßÒÍÎÅ ÐÀÑ×ÅÒÍÎÅ ÑÐÅÄÍÅÅ ÇÀ ÏÅÐÈÎÄ ÇÍÀ×ÅÍÈÅ ÎÒÍÎÑÈÒÅËÜÍÎÃÎ ×ÈÑËÀ ÑÎËÍÅ×ÍÛÕ ÏßÒÅÍ Â ÌÅÆÄÓÍÀÐÎÄÍÎÉ ÑÈÑÒÅÌÅ W=050+10/-10. ...
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Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110321.txt -- 5.2 Êá -- 21.03.2011
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1386. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110314.txt
... ÏÎ ÄÀÍÍÛÌ Ñ ÊÎÐÎÍÎÃÐÀÔΠÑÎÕÎ ÄÎ 8 ÌÀÐÒÀ ÍÀÁËÞÄÀËÈÑÜ 25 ÊÎÐÎÍÀËÜÍÛÕ ÂÛÁÐÎÑΠÂÅÙÅÑÒÂÀ, ÒÐÈ ÈÇ ÊÎÒÎÐÛÕ ÁÛËÈ ÊËÀÑÑÀ ×ÀÑÒÈ×ÍÎÅ ÃÀËÎ . --------------------------------------------------------------------- to tm te êîî-òû áàëë Å(1-8A) ÀÎ RII/IV CME ðåíò îï J/m-2 Mãö 07.03 /0502 0513 0525 N24W48L162 M1.2/1F 8.1E-3 11164 07.03 /0759 0807 0828 N27W47L162 M1.4/1F 1.0E-2 11164 07.03 /0749 0754 0803 S20W78L181 M1.5/SF 3.7E-3 11165 ... ÝÒÈ ÃÅÎÌÀÃÍÈÒÍÛÅ ÂÎÇÌÓÙÅÍÈß ÂÛÇÂÀÍÎ ÑÅÐÈÅÉ ÂÑÏÛØÅÊ 7-9 ÌÀÐÒÀ. ...
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Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110314.txt -- 6.8 Êá -- 14.03.2011
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1387. http://www.izmiran.rssi.ru/~obridko/papers/412.pdf
... Open Magnetic Fields on the Sun and Solar Wind Parameters at the Earth's Orbit V. N. Obridko*, B. D. Shelting, and I. M. Livshits Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radio Wave ... Region, 142190 Russia Received August 19, 2010; in final form, September 20, 2010 Abstract--It is shown that the parameters of the solar -wind magnetic field are determined by regions in coronal holes at distances of 1.1´1.4 ... 3 2011 OPEN MAGNETIC FIELDS ON THE SUN 10. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/412.pdf -- 585.1 Êá -- 14.03.2011
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1388. http://www.izmiran.rssi.ru/~obridko/papers/386engl.pdf
... 86, No. 11, pp. 1125´1132. i Relationship between the Contrast of Coronal Holes and Parameters of the Solar Wind Streams V. N. Obridko1, B. D. Shelting1 , I. M. Livshits1 , and A. B. Askerov 1 2 2 Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow oblast, 142190 Russia Shemakha Astrophysical Observatory, National Academy of Sciences of Azerbaijan Republic, Yu. ... This value may differ significantly from the mean...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/386engl.pdf -- 793.7 Êá -- 14.03.2011
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1389. http://www.izmiran.rssi.ru/~obridko/papers/358.pdf
... Three prediction indices have been proposed: the intensity of the polar field, the mean field at the source surface, and a recurrence index of geomagnetic disturbances. ... However, the cyclic variation of geomagnetic activity is controlled by the large-scale solar fields (Obridko and Shelting, 1992; Belov, Obridko, and Shelting, 2006). ... Having obtained the magnetic field expansion coefficients, one can calculate the polar field at any height (Obridko and Shelting, 1999). ... Solar-Terr. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/358.pdf -- 506.2 Êá -- 14.03.2011
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1390. http://www.izmiran.rssi.ru/~obridko/papers/355.pdf
... It has been established that the transition from the background magnetic field to the fields of an active region occurs near 25´50 G. A dependence of the exponent H on the magnetic field amplitude has been derived. The exponent H for the background magnetic field has been found to be much smaller than that for the fields of an active region. ... Fig. ... As follows from the estimates of Fig. 3, the exponent H is 0.5´0.7 for the magnetic fields of an active region and 0.1 for the background field. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/355.pdf -- 614.6 Êá -- 14.03.2011
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1391. http://www.izmiran.rssi.ru/~obridko/papers/354.pdf
Advances in Space Research 40 (2007) 1006-1014 www.elsevier.com/locate/asr Occurrence of the 1.3-year periodicity in the large-scale solar magnetic field for 8 solar cycles V.N. Obridko *, B.D. Shelting Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Russian Academy of Sciences, ... Region 142190, Russia Received 23 October 2006; received in revised form 26 February 2007; accepted 10 April 2007 Abstract The data on ... 1998; Anan'ev and Obridko, 1999). ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/354.pdf -- 864.8 Êá -- 14.03.2011
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1392. http://www.izmiran.rssi.ru/~obridko/papers/353.pdf
... 84, No. 4, pp. 380´384. i A Generalized Polarity Rule for Solar Magnetic Fields V. N. Obridko and B. D. Shel'ting Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences ... 142190 Russia Received August 23, 2006; in final form, October 12, 2006 Abstract--It is shown that, when all components of the large-scale solar magnetic field are longitudinally averaged, the N ... The large-scale fields spread all over the solar surface. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/353.pdf -- 161.7 Êá -- 14.03.2011
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1393. http://www.izmiran.rssi.ru/~obridko/papers/352engl.pdf
... We show that the correlation between the intensity of the coronal Fe XIV 530.5 nm green line and the calculated magnetic field strength in the solar corona can be a useful tool for this purpose. ... In this paper, we compare the observed patterns of correlation between the coronal green line intensity and the magnetic field strength in various latitude zones with the results of theoretical calculations for several solar coronal heating models. ... In contrast, the green line intensity is very low. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/352engl.pdf -- 650.7 Êá -- 14.03.2011
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1394. http://www.izmiran.rssi.ru/~obridko/papers/351.pdf
... 2003, 2005; Badalyan, Obridko, and SÙkora, 2005b) the following topics were treated: (1) The space ´ time distributions of the N ´ S asymmetry derived from different solar activity indices and their mutual correlations on both short and long time scales (2) Quasi-biennial oscillations ( QBO ) in the N ´ S asymmetry of the activity indices and their space ´ time distribution and comparison of the QBO in the N ´ S ... Figure 4 The time profiles of SVAN amplitudes shown in Figure...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/351.pdf -- 802.4 Êá -- 14.03.2011
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1395. http://www.izmiran.rssi.ru/~obridko/papers/350.pdf
Solar Physics (2006) 238: 271´292 DOI: 10.1007/s11207-006-0214-2 C Springer 2006 TWO REGULARITIES IN THE CORONAL GREEN-LINE BRIGHTNESS ´ MAGNETIC FIELD COUPLING AND THE HEATING OF THE CORONA O.G. BADALYAN and V.N. OBRIDKO Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, 142190 Troitsk, Moscow, Russia (e-mail: badalyan@izmiran.troitsk.ru) (Received 27 April 2006; accepted 20 August 2006; Published online 14 October 2006) Abstract. ... 30 and the zone above | ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/350.pdf -- 839.5 Êá -- 14.03.2011
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1396. http://www.izmiran.rssi.ru/~obridko/papers/348rus.pdf
... 1?ßiÛÜâÝfl ðÑë~ÒÜã âäÒÒÞÒÜÛÒ ß,, ÜÛêÜã ,,ã äãÞfl âãÞÜÒ ~Üã,,ã ,Òê ,ÇÞÛÑÛ ñÒßÞÛ Û âãäãâê,ÞÒÜã â êÒß, ~êã ãÚÛÞãâÈ äã ÝÞââÛ~ÒâÝãØ ßãÒÞÛ. øãÝÑÜã, ~êã ,ëi,Ò?ÛÜÜãâêÈ âäÒÒÞÒÜÛfl ÑÜ~ ÒÜÛØ ßÒÚäÞÜÒêÜã,,ã ß,, ÜÛêÜã ,,ã äãÞfl , ãÇÜëÚÒÜÜfl ÜÒÒ, ÜÒ fl,ÞflÒêâfl êÒéÝêãß ëâÒÜÒÜÛfl, ãêÚÒê ÒÞÈÜë âêëÝêëë ß,, ÜÛêÜã ,,ã äãÞfl ,ÜëêÛ âÒÝêã. øÛ êãß ÇãÞÒÒ ~âêã ,âêÒ~Òêâfl ß,,ÜÛêÜãÒ äãÞÒ äãÞflÜãâêÛ, ... ÕãÞÒÒ êã,,ã ,,Ûâêã,,ßß âêÞ ?ÛÒ Û ÑÜ~ÒÜÛfl ßÝâÛßëßã, (äÛÝã,) Ü Û,,ßßÒ âÒÜÒ~âã,Ài ÑÜ~ÒÜÛØ âããê,Òêâê,ëê Á4.5 ÜýÞ. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/348rus.pdf -- 225.3 Êá -- 14.03.2011
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1397. http://www.izmiran.rssi.ru/~obridko/papers/348engl.pdf
... Magnetic Cloud in the Solar Wind : A Comparison with the Classical Model A. B. Askerova and V. N. Obridkob b Shemakha Astrophysical Observatory, Academy of Sciences ... Academy of Sciences, Troitsk, Moscow oblast, 142190 Russia Received March 20, 2006; in final form, November 1, 2006 a Abstract--The solar wind magnetic field distribution near the Earth has been studied and compared with the distribution anticipated according to the classical model ... Fig. ... values. ... 2007 Fig. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/348engl.pdf -- 288.5 Êá -- 14.03.2011
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1398. http://www.izmiran.rssi.ru/~obridko/papers/347engl.pdf
... 83, No. 11, pp. 1031´1041. i Variations of the Dipole Magnetic Moment of the Sun during the Solar Activity Cycle I. M. Livshits and V. N. Obridko Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radiowave Propagation, Troitsk, Russia Received February 28, 2006; in final form, March 13, 2006 Abstract--Observations of the large-scale solar magnetic field (synoptic maps) and measurements of the magnetic ... A 100 000 10 000 10 20 30 40 50 60 Period, days Fig. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/347engl.pdf -- 629.2 Êá -- 14.03.2011
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1399. http://www.izmiran.rssi.ru/~obridko/papers/328rus.pdf
... Ñ ÝÚÀØ ÒÜÈ ââ~ÛêÜã âãÞÜÒ ~ÜãÒ ß,,ÜÛêÜãÒ äãÞÒ Bs Þfl äãÒÝ^ÛÛ ñÒßÞÛ Ü äã,ÒiÜãâêÈ Ûâêã~ÜÛÝ âãÞÜÒ ~Üã,,ã ,Òê. ?êÛ ÜÜÀÒ âãäãâê,ÞflÞÛâÈ âã âÒÜÒâëêã~ÜÀßÛ ÑÜ~ÒÜÛflßÛ âÝããâêÛ âãÞÜÒ ~Üã,,ã ,Òê Û ÑÞÛ~ÜÀßÛ ÝãßäãÜÒÜêßÛ ßÒÚäÞÜÒêÜã,,ã ß,, ÜÛêÜã ,,ã äãÞfl ë ñÒßÞÛ . ûêêÛâêÛ~ÒâÝÛØ ÜÞÛÑ ,Àfl,ÛÞ ãâêêã~Üã êÒâÜë â,flÑÈ ßÒÚë iÝêÒÛâêÛÝßÛ âãÞÜÒ ~Üã,,ã ,Òê ë ûãÞÜ^ Û ë ñÒßÞÛ , äÒÛãÀ ÇÒÑ ÑÜ~ÛêÒÞÈÜÀi âäãÛ~ÒâÝÛi âãÞÜÒ ~ ... Ûâ. 6). ôÝ Û ÜÒÒ Þfl âÝããâêÛ âãÞÜÒ~Üã,,ã ,Òê, Þfl äãâêãÒÜÛfl Ûâ. ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/328rus.pdf -- 370.3 Êá -- 14.03.2011
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1400. http://www.izmiran.rssi.ru/~obridko/papers/328engl.pdf
... Correlation between the Near-Earth Solar Wind Parameters and the Source Surface Magnetic Field A. V. Belov, V. N. Obridko, and B. D. Shelting Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences, Troitsk, Moscow oblast, 142190 Russia Received February 16, 2005 Abstract--The solar magnetic field Bs at the Earth's projection onto the solar-wind source surface has been calculated for each day over a long time interval (1976´2004). ...
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Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/328engl.pdf -- 241.6 Êá -- 14.03.2011
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