Ïîèñê ïî:www.izmiran.rssi.ru -
Ïîèñêàòü ïî âñåì ñåðâåðàì
Íà ýòîé ñòðàíèöå ïðèâåäåíû âñå ñòðàíèöû ñåðâåðà www.izmiran.rssi.ru ,êîòîðûå ìû èíäåêñèðóåì. Ïîêàçàíû äîêóìåíòû 1361 - 1380 èç 2408.
Óïîðÿäî÷èòü ïî:
URL
|
äàòå èçìåíåíèÿ
1361. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110523.txt
ÎÁÇÎÐ ÑÎÑÒÎßÍÈß ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ, ÃÅÎÝÔÔÅÊÒÈÂÍÛÕ ßÂËÅÍÈÉ È ÈÕ ÂÎÇÄÅÉÑÒÂÈÉ ÍÀ ÎÊÎËÎÇÅÌÍÎÅ ÊÎÑÌÈ×ÅÑÊÎÅ ÏÐÎÑÒÐÀÍÑÒÂÎ ÍÀ ÏÅÐÈÎÄ 16 - 22.05.2011 ã. È ÏÐÎÃÍÎÇ ÍÀ 23 - 30.05.2011 ã. ÊÝÐÐÈÍÃÒÎÍÎÂÑÊÈÉ ÎÁÎÐÎÒ 2110 (09,60.05.2011) ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÀß ÀÊÒÈÂÍÎÑÒÜ ÑÎËÍÖÀ ÏÐÎØÅÄØÅÃÎ ÏÅÐÈÎÄÀ ÄÅÐÆÀËÀÑÜ ÍÀ ÑÐÅÄÍÅÌ, À 19 ÌÀß ÍÀ ÍÈÇÊÎÌ ÓÐÎÂÍÅ. ... ÍÀ ÑËÅÄÓÞÙÅÉ ÍÅÄÅËÅ ÓÐÎÂÅÍÜ ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÎÆÈÄÀÅÒÑß ÍÈÇÊÈÌ È ÑÐÅÄÍÈÌ. ... ÂÑÏÛØÅ×ÍÀß ÀÊÒÈÂÍÎÑÒÜ ÁÛËÀ ÍÀ ÍÈÇÊÎÌ ÓÐÎÂÍÅ ÒÎËÜÊÎ 18 ÌÀß. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110523.txt -- 4.6 Êá -- 23.05.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1362. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110516.txt
ÎÁÇÎÐ ÑÎÑÒÎßÍÈß ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ, ÃÅÎÝÔÔÅÊÒÈÂÍÛÕ ßÂËÅÍÈÉ È ÈÕ ÂÎÇÄÅÉÑÒÂÈÉ ÍÀ ÎÊÎËÎÇÅÌÍÎÅ ÊÎÑÌÈ×ÅÑÊÎÅ ÏÐÎÑÒÐÀÍÑÒÂÎ ÍÀ ÏÅÐÈÎÄ 09 - 15.05.2011 ã. È ÏÐÎÃÍÎÇ ÍÀ 16 - 23.05.2011 ã. ÊÝÐÐÈÍÃÒÎÍÎÂÑÊÈÉ ÎÁÎÐÎÒ 2009, 2110 (12,35.04; 09,60.05.2011) ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÀß ÀÊÒÈÂÍÎÑÒÜ ÑÎËÍÖÀ ÏÐÎØÅÄØÅÃÎ ÏÅÐÈÎÄÀ ÄÅÐÆÀËÀÑÜ ÍÀ ÑÐÅÄÍÅÌ, À 12-13 ÌÀß ÍÀ ÍÈÇÊÎÌ ÓÐÎÂÍÅ. ... ÍÀ ÑËÅÄÓÞÙÅÉ ÍÅÄÅËÅ ÓÐÎÂÅÍÜ ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÎÆÈÄÀÅÒÑß ÍÈÇÊÈÌ È ÑÐÅÄÍÈÌ. ... ÂÑÏÛØÅ×ÍÀß ÀÊÒÈÂÍÎÑÒÜ ÁÛËÀ ÍÀ ÍÈÇÊÎÌ ÓÐÎÂÍÅ 9 È 12 ÌÀß. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110516.txt -- 4.6 Êá -- 16.05.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1363. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110509.txt
ÎÁÇÎÐ ÑÎÑÒÎßÍÈß ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ, ÃÅÎÝÔÔÅÊÒÈÂÍÛÕ ßÂËÅÍÈÉ È ÈÕ ÂÎÇÄÅÉÑÒÂÈÉ ÍÀ ÎÊÎËÎÇÅÌÍÎÅ ÊÎÑÌÈ×ÅÑÊÎÅ ÏÐÎÑÒÐÀÍÑÒÂÎ ÍÀ ÏÅÐÈÎÄ 02 - 08.05.2011 ã. È ÏÐÎÃÍÎÇ ÍÀ 09 - 16.05.2011 ã. ÊÝÐÐÈÍÃÒÎÍÎÂÑÊÈÉ ÎÁÎÐÎÒ 2109 (12,35.04.2011) ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÀß ÀÊÒÈÂÍÎÑÒÜ ÑÎËÍÖÀ ÏÐÎØÅÄØÅÃÎ ÏÅÐÈÎÄÀ  ÎÑÍÎÂÍÎÌ ÄÅÐÆÀËÀÑÜ ÍÀ ÑÐÅÄÍÅÌ ÓÐÎÂÍÅ ÑÎ ÑÏÀÄÎÌ ÄÎ ÍÈÇÊÎÃÎ 07 ÌÀß. ... ÍÀ ÑËÅÄÓÞÙÅÉ ÍÅÄÅËÅ ÓÐÎÂÅÍÜ ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÎÆÈÄÀÅÒÑß ÍÈÇÊÈÌ È ÑÐÅÄÍÈÌ. ... ÂÑÏÛØÅ×ÍÀß ÀÊÒÈÂÍÎÑÒÜ ÁÛËÀ ÍÀ ÍÈÇÊÎÌ ÓÐÎÂÍÅ 2 È 3 ÌÀß. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110509.txt -- 5.0 Êá -- 09.05.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1364. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110502.txt
ÎÒÍÎÑÈÒÅËÜÍÎÅ ×ÈÑËÎ ÏßÒÅÍ Â ÀÏÐÅËÅ 2011 ã. ÑÎÑÒÀÂÈËÎ - Wàïð. 54.4, ×ÒÎ ÄÀÅÒ ÄËß 22 ÌÅÑßÖÀ (ÎÊÒßÁÐÜ 2010 ã.) ÐÀÇÂÈÒÈß ÒÅÊÓÙÅÃÎ 24 ÖÈÊËÀ ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÑÃËÀÆÅÍÍÎÅ ×ÈÑËÎ ÂÎËÜÔÀ - W*ñåí. ... ÍÀ ÑËÅÄÓÞÙÅÉ ÍÅÄÅËÅ ÓÐÎÂÅÍÜ ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÎÆÈÄÀÅÒ- Ñß ÑÐÅÄÍÈÌ È ÂÛÑÎÊÈÌ. ... ÃÅÎÌÀÃÍÈÒÍÀß ÎÁÑÒÀÍÎÂÊÀ ÁÛËÀ ÂÎÇÌÓÙÅÍÍÎÉ ÒÎËÜÊÎ 29-30 ÀÏÐÅËß, ÊÎÃÄÀ ÏÎ ÄÀÍÍÛÌ ÇÀÏÀÄÍÛÕ ÑÒÀÍÖÈÉ ÇÀÐÅÃÈÑÒÐÈÐÎÂÀÍÀ ÌÀËÀß ÌÀÃÍÈÒÍÀß ÁÓÐß (G1, Ams= 23,äëèò.=30 ÷.). ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110502.txt -- 5.8 Êá -- 02.05.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1365. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110425.txt
ÎÁÇÎÐ ÑÎÑÒÎßÍÈß ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ, ÃÅÎÝÔÔÅÊÒÈÂÍÛÕ ßÂËÅÍÈÉ È ÈÕ ÂÎÇÄÅÉÑÒÂÈÉ ÍÀ ÎÊÎËÎÇÅÌÍÎÅ ÊÎÑÌÈ×ÅÑÊÎÅ ÏÐÎÑÒÐÀÍÑÒÂÎ ÍÀ ÏÅÐÈÎÄ 18 - 24.04.2011 ã. È ÏÐÎÃÍÎÇ ÍÀ 25.04 - 02.05.2011 ã. ÊÝÐÐÈÍÃÒÎÍÎÂÑÊÈÉ ÎÁÎÐÎÒ 2109 (12,35.04.2011) ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÀß ÀÊÒÈÂÍÎÑÒÜ ÑÎËÍÖÀ ÏÐÎØÅÄØÅÃÎ ÏÅÐÈÎÄÀ  ÎÑÍÎÂÍÎÌ ÄÅÐÆÀËÀÑÜ ÍÀ ÑÐÅÄÍÅÌ ÓÐÎÂÍÅ. ... ÐÀÑ×ÅÒÍÎÅ, ÑÐÅÄÍÅÅ ÇÀ ÏÅÐÈÎÄ ÇÍÀ×ÅÍÈÅ ÎÒÍÎÑÈÒÅËÜÍÎÃÎ ×ÈÑËÀ ÑÎËÍÅ×ÍÛÕ ÏßÒÅÍ Â ÌÅÆÄÓÍÀÐÎÄÍÎÉ ÑÈÑÒÅÌÅ ÑÎÑÒÀÂÈËÎ W=051+11/-11. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110425.txt -- 5.6 Êá -- 25.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1366. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110418.txt
... Îáå ÊÄ - çàëèâÛ þæíîé ïîëÿðíîé äûðû. ... ÀÏÐÅËÜ 02 03 04 05 06 07 08 09 ÀÏÐÅËÜ Wus 066 070 083 065 056 073 097 056 F10.7 108 114 113 109 117 112 109 105 Õbcg Â2.2 Â3.9 B3.3 B2.8 B3.1 B3.1 Â2.6 Â2.9 GOES Sp 280 290 340 380 230 290 330 150 Nnew 1 1 1 2 IMF - - - - - - - - ACE å 2 8.9Å+6 3.7Å+8 1.3Å+9 1.2E+9 2.7Å+7 5.4Å+6 1.1Å+7 9.6Å+6 GOES Nm% THULE Ap 20 16 8 7 26 6 8 10 Àð Dst ÊÈÎÒÎ Amsc 14 10 8 20 11 11 10 ÈÇÌÈÐÀÍ ----------------------------------------------------------------------- ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110418.txt -- 6.8 Êá -- 18.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1367. http://www.izmiran.rssi.ru/~obridko/papers/252.pdf
instructions for authors and subscription information: http://www.informaworld.com/smpp/title~content=t713453505 Quasi-biennial oscillations of the solar global magnetic field B. D. Shelting a; V. N. Obridko a a Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, RAS, Moscow Region, Russia Online Publication Date: 01 October 2001 To cite this Article: Shelting , B. D. and Obridko , V. N. (2001) 'Quasi-biennial ... This means that QBO have a global nature. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/252.pdf -- 491.4 Êá -- 07.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1368. http://www.izmiran.rssi.ru/~obridko/papers/407.pdf
... 357í365 Contents lists available at ScienceDirect New Astronomy journal h omepage: www.else vier.com/locate/newast NorthíSouth asymmetry of the sunspot indices and its quasi-biennial oscillations O.G. Badalyan , V.N. Obridko Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, 142190 Troitsk, Russia article info abstract The spaceítime distribution of asymmetry in the area and total number of ... Sunspots and Activity Complexes. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/407.pdf -- 820.1 Êá -- 07.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1369. http://www.izmiran.rssi.ru/~obridko/papers/313.pdf
including instructions for authors and subscription information: http://www.informaworld.com/smpp/title~content=t713453505 Space- time distributions of the coronal green-line brightness and solar magnetic fields O. G. Badalyan a; V. N. Obridko a; J. SÙkora b a Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Troitsk, Russia b Astronomical ... Characteristic CGLB synoptic charts for cycle 21. ... SPACE´TIME DISTRIBUTIONS OF CGLB AND SOLAR MAGNETIC FIELDS Table 2. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/313.pdf -- 827.5 Êá -- 07.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1370. http://www.izmiran.rssi.ru/~obridko/papers/320.pdf
... Figure 1a illustrates the summary diagram (2 log L, log S ) based on the field intensity contour lines for 7 active regions plotted at 200 G steps in the range of 2200´400 G. One can see that the relationship under discussion is well represented by two straight lines, one corresponding to the log S range from 2 to 7.2 and another, from 7.2 to 9. ... Then, we plotted 2 log L versus log S for all field lines of a given intensity, no matter which sunspot or sunspot group they belonged to. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/320.pdf -- 77.9 Êá -- 07.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1371. http://www.izmiran.rssi.ru/~obridko/papers/202.pdf
... The daily measurements of the group (27 persons) have shown the presence of a synchronous mass response of inspected people on magnetic storms. ... 6) The phase of hyperfunction is not registered, but a phase of depression is clearly visible. (c) 50% of inspected people have reacted to the sharp jump of the geomagnetic field as in a storm. (d) Response to jumps of atmospheric pressure is characterized by the absence of the phase of depression. ... 1992) The Physiological Active VLF Magnetic Fields. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/202.pdf -- 813.0 Êá -- 07.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1372. http://www.izmiran.rssi.ru/~obridko/papers/149.pdf
... Moreover, it even seems at all doubtful that solar wind velocity variations be mainly determined by the field structure in the Sun. ... The solar wind velocity values, V,, obtained by Wang and Sheeley (1990) from the expansion factor, f,, are: V, 650 km/s 650 km/s 2 V, 550 km/s 550 km/s 2 V, 450 km/s 450 km/s 2 V, f, 3.5 3.5 5 9.0 9.0 5 f, 18.0 fJ 18.0 _ f, THE SOLAR WIND PARAMETERS The histopam of relation between the measured velocities and the velocities Table 1...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/149.pdf -- 690.1 Êá -- 07.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1373. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110402.txt
... ÎÒÍÎÑÈÒÅËÜÍÎÅ ×ÈÑËÎ ÏßÒÅÍ Â ÔÅÂÐÀËÅ 2011 ã. ÑÎÑÒÀÂÈËÎ - Wìàðò =56.2, ×ÒÎ ÄÀÅÒ ÄËß 21 ÌÅÑßÖÀ (ÑÅÍÒßÁÐÜ 2010 ã.) ÐÀÇÂÈÒÈß ÒÅÊÓÙÅÃÎ 24 ÖÈÊËÀ ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÑÃËÀÆÅÍÍÎÅ ×ÈÑËÎ ÂÎËÜÔÀ - W*ñåí. ... ÌÈÍÈÌÓÌ 23 ÑÎËÍÅ×ÍÎÃÎ ÖÈÊËÀ - ÄÅÊÀÁÐÜ 2008 ã. - W*=1.7. ... ÍÀ ÂÈÄÈÌÎÌ ÄÈÑÊÅ ÑÎËÍÖÀ ÏÎÑÒÎßÍÍÎ ÎÒ ØÅÑÒÈ ÄÎ ×ÅÒÛÐÅÕ ÍÅÁÎËÜØÈÕ ÃÐÓÏÏ ÑÎËÍÅ×ÍÛÕ ÏßÒÅÍ, ÓÌÅÍÜØÀßÑÜ Ê ÊÎÍÖÓ ÏÅÐÈÎÄÀ. ÍÀ ÑËÅÄÓÞÙÅÉ ÍÅÄÅËÅ ÓÐÎÂÅÍÜ ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÎÉ ÀÊÒÈÂÍÎÑÒÈ ÎÆÈÄÀÅÒ- Ñß ÑÐÅÄÍÈÌ È ÂÛÑÎÊÈÌ. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110402.txt -- 6.3 Êá -- 02.04.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1374. http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110328.txt
ÎÁÇÎÐ ÑÎÑÒÎßÍÈß ÑÎËÍÅ×ÍÎÉ ÀÊÒÈÂÍÎÑÒÈ, ÃÅÎÝÔÔÅÊÒÈÂÍÛÕ ßÂËÅÍÈÉ È ÈÕ ÂÎÇÄÅÉÑÒÂÈÉ ÍÀ ÎÊÎËÎÇÅÌÍÎÅ ÊÎÑÌÈ×ÅÑÊÎÅ ÏÐÎÑÒÐÀÍÑÒÂÎ ÍÀ ÏÅÐÈÎÄ 21 - 27.03.2011 ã. È ÏÐÎÃÍÎÇ ÍÀ 28 - 03.03.2011 ã. ÊÝÐÐÈÍÃÒÎÍÎÂÑÊÈÉ ÎÁÎÐÎÒ 2108 (16,06.03.2011) ÏßÒÍÎÎÁÐÀÇÎÂÀÒÅËÜÍÀß ÀÊÒÈÂÍÎÑÒÜ ÑÎËÍÖÀ ÏÐÎØÅÄØÅÃÎ ÏÅÐÈÎÄÀ ÏÎÄÍÈÌÀËÀÑÜ ÎÒ ÍÈÇÊÎÃÎ ÄÎ ÂÛÑÎÊÎÃÎ ÓÐÎÂÍÅÉ. ÐÀÑ×ÅÒÍÎÅ, ÑÐÅÄÍÅÅ ÇÀ ÏÅÐÈÎÄ ÇÍÀ×ÅÍÈÅ ÎÒÍÎÑÈÒÅËÜÍÎÃÎ ×ÈÑËÀ ÑÎËÍÅ×ÍÛÕ ÏßÒÅÍ Â ÌÅÆÄÓÍÀÐÎÄÍÎÉ ÑÈÑÒÅÌÅ ÑÎÑÒÀÂÈËÎ W=054+26/-35. ...
[
Ñîõðàíåííàÿ êîïèÿ
]
Ññûëêè http://www.izmiran.rssi.ru/services/saf/archive/ru/2011/obzor20110328.txt -- 5.4 Êá -- 28.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1375. http://www.izmiran.rssi.ru/~obridko/papers/128.pdf
CYCLIC VARIATION OF THE GLOBAL MAGNETIC FIELD INDICES V. N. OBRIDKO andB. ... The energetical aspect of solar phenomena of different spatial and time scales has been studied with special attention to global magnetic fields, Cyclic regularities in the heliosphere are determined by energetics of global magnetic fields. ... Introduction The cyclic variation of solar activity is usually characterized by special indices associated with local magnetic fields. ... One Solar Physics 137: 167-177, 1992. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/128.pdf -- 596.6 Êá -- 22.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1376. http://www.izmiran.rssi.ru/~obridko/papers/35.pdf
BARTELS' ACTIVE LONGITUDES', SECTOR BOUNDARIES AND FLARE ACTIVITY V. BUMBA and V. N. OBRIDKO* Astronomical Institute of the Czechoslovak Academy of Sciences, Ond(ejov (Received 27 June, 1968) Abstract. The flare activity and especially the proton-flare activity is concentrated in the zones of 'Bartels' active longitudes' and in the neighbourhood closest to the sector boundaries of the interplanetary magnetic field. ... TABLE I CMP of proton-flare groups and sector boundaries. ... BUMBA, Active 56. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/35.pdf -- 397.6 Êá -- 22.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1377. http://www.izmiran.rssi.ru/~obridko/papers/33.pdf
LARGE-SCALE MUTUAL RELATIONS OF SPOT GROUPS IN PROTON COMPLEX L. KRIVSK~ and V. OBRIDKO* Astronomical Institute of the Czechoslovak Academy of Sciences, Ondfejov (Received 20 May, 1968; revision received 1 August, 1968) Abstract. ... The probability of occurrence of accompanying spot groups (satellites) was studied according to the classification types, the direction of their occurrence, and the distance with respect to the proton spot group. ... Results A. PROTON GROUP TYPE AND SATELLrI'I.~ TYP}! ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/33.pdf -- 478.5 Êá -- 22.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1378. http://www.izmiran.rssi.ru/~obridko/papers/142.pdf
SOME COMMENTS ON THE PROBLEM OF SOLAR CYCLE PREDICTION V. N. OBRIDKO IZMIRAN, Troitsk, Moscow Region 142092, Russia (Received 26 November, 1993; in revised form 8 September, 1994) Abstract. The paper provides a number of regression equations that can be used to calculate the height of the odd Wolf number cycle. ... 1) Solar Physics 156: 179-190, 1995. ... 2) We introduce an index, a(RM), that is the ratio of the maximum annual mean Wolf numbers in the odd-following and the even cycles in a pair. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/142.pdf -- 636.2 Êá -- 22.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1379. http://www.izmiran.rssi.ru/~obridko/papers/46.pdf
... Correlation analysis applied to recordings of the magnetic field and velocity of the Sun as a star reveals oscillations close to 300 s. The power spectrum of these oscillations is discussed. ... The power spectrum for the magnetic field has a wide maximum in the interval 580-200 s with peak at 390 s. The maxima of the power spectrum for the radial velocities correspond to 50 and 80 s. The curves for the second period of observation, May 20th, are presented in Figure 3. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/46.pdf -- 278.0 Êá -- 22.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû
1380. http://www.izmiran.rssi.ru/~obridko/papers/218.pdf
AMPLITUDE AND PERIOD OF THE DYNAMO WAVE AND PREDICTION OF THE SOLAR CYCLE ISABELLA V. DMITRIEVA, KIRILL M. KUZANYAN and VLADIMIR N. OBRIDKO IZMIRAN, Troitsk, Moscow Region, 142190 Russia (e-mails: bella@izmiran.troitsk.ru; kuzanyan@dnttm.ru; solter@izmiran.troitsk.ru) (Received 5 October 1999; accepted 8 March 2000) Abstract. ... This means that we may try to predict the average amplitude of a given solar cycle by knowing the derivative of the Wolf numbers within previous periods. ...
[
Òåêñò
]
Ññûëêè http://www.izmiran.rssi.ru/~obridko/papers/218.pdf -- 105.1 Êá -- 22.03.2011
Ïîõîæèå äîêóìåíòû
Ïîõîæèå äîêóìåíòû