It looks like you're offline.
Open Library logo
additional options menu

MARC Record from marc_columbia

Record ID marc_columbia/Columbia-extract-20221130-012.mrc:110314444:6793
Source marc_columbia
Download Link /show-records/marc_columbia/Columbia-extract-20221130-012.mrc:110314444:6793?format=raw

LEADER: 06793cam a2200373Ia 4500
001 5618441
005 20221121194458.0
008 060221t20052005caua b 101 0 eng d
010 $a 2005936501
020 $a1583812148
035 $a(OCoLC)ocm64178673
035 $a(NNC)5618441
035 $a5618441
040 $aSTI$cSTI$dOrLoB-B
043 $azsu----
050 00 $aQB526.A37$bN37 2004
110 2 $aNational Solar Observatory/Sacramento Peak.$bSummer Workshop$n(22nd :$d2004 :$cSunspot, N.M.)
245 10 $aLarge-scale structures and their role in solar activity :$bproceedings of the 22nd Sacramento Peak Workshop, held at the National Solar Observatory, Sacramento Peak, Sunspot, New Mexico, USA, 18-22 October 2004 /$cedited by K. Sankarasubramanian, Matt Penn, and Alexei Pevtsov.
250 $a1st ed.
260 $aSan Francisco, Calif. :$bAstronomical Society of the Pacific,$c[2005], ©2005.
300 $axiv, 432 pages :$billustrations ;$c24 cm.
336 $atext$btxt$2rdacontent
337 $aunmediated$bn$2rdamedia
490 1 $aAstronomical Society of the Pacific conference series ;$vv. 346
504 $aIncludes bibliographical references and index.
505 00 $tLarge-scale transport of magnetic flux and flows in solar convection zone /$rP. Ambroz -- $tHow large-scale flows may influence solar activity /$rD. Hathaway -- $tLarge-scale flows in subsurface layers /$rR. Komm, R. Howe, I. Gonzalez Hernandez, F. Hill and C. Toner -- $tPhotospheric surface flows and sunspot moats /$rM. Hagenaar -- $tOn the characteristic scales of solar convection /$rR. Sridharan -- $tCALAS, a camera for the large-scale of the solar surface /$rN. Meunier, S. Rondi, R. Tkaczuk, M. Rieutord and F. Beigbeder -- $tLarge-scale organization in the solar dynamo and its observational signature /$rM. Dikpati -- $tFighting the Taylor-Proudman constraint - how to get differential rotation solar-like? /$rM. Rempel -- $tWhat does the solar differential rotation tell us about large-scale waves? /$rE. Kaghashvilii, G. Webb and G. Zank -- $tCoherent structures vs independent modes of the axisymmetric magnetic field fluctuations /$rA. Cadavid, J. Lawrence, D. McDonald and A. Ruzmaikin -- $tHow sensitive are rotation inversions to subtle features of the dynamo? /$rR. Howe, M. Rempel, J. Christensen-Dalsgaard, J. Schou, M. Thompson, R. Komm and F. Hill -- $tInfluence of depth-dependent diffusivity profiles in governing the evolution of weak, large-scale magnetic fields of the sun /$rE. Zita, N. Song, E. McDonald and M. Dikpati -- $tJets in the solar tachocline as diagnostics of global MHD processes /$rJ. Christensen-Dalsgaard, T. Cobard, M. Dikpati, P. Gilman and M. Thompson -- $tThe formation and evolution of complexes of activity, activity nests, and the large-scale connectivity in the solar corona /$rE. Benevolenskaya -- $tCoronal emission lines linear polarization : a tracer of coronal magnetic fields topology /$rJ. Arnaud -- $tLow frequency (< 100MHz) thermal radio emission from the solar corona and the effect of radial magnetic field /$rR. Ramesh and Ch. Sastry -- $tLarge-scale non-axisymmetric magnetic fields on the sun and cool stars /$rS. Berdyugina -- $tInterpretation of solar and stellar activity in terms of dynamo modes /$rD. Fluri and S. Berdyugina -- $tRole of large-scale magnetic fields and material flows in the formation of filaments and filament channels /$rD. Mackay -- $tMotions and interactions among large-scale solar structures on H-alpha synoptic charts /$rP. McIntosh -- $tFormation of an extraordinarily long filament channel /$rM. Anderson and S. Martin -- $tThe internal structures and dynamics of solar quiescent prominences /$rG. Petrie and B. Low -- $tAccumulation of filament material at the boundaries of supergranular cells /$rA. Pevtsov and D. Neidig -- $tMagnetic fields and flows in open magnetic structures /$rH. Jones -- $tRadio and EUV measurements of the equatorial coronal hole of February 25, 1999 /$rK. Subramanian and G. Shanmugha Sundaram -- $tMulti-wavelength observations of coronal holes /$rG. de Toma and C. Arge -- $tAutomated coronal hole detection using He I 1083 nm spectroheliograms and photospheric magnetograms /$rC. Henney and J. Harvey -- $tThe chromospheric prolateness and its variations /$rJ. Vilinga and S. Koutchmy -- $tMagnetic field reversal of the sun in polarization of radio emission at 17GHz /$rA. Tlatov, G. Gelfreikh and V. Makarov -- $tLarge-scale organizations related to eruptive phenomena on the solar surface /$rJ. Lin -- $tOn magnetic structures of solar active regions and geomagnetic storms /$rY. Liu -- $tMultiple large-scale MHD shocks related radio emission at decameter wavelengths /$rE. Ebenezer -- $tGenesis of AR NOAA10314 /$rS. Morita and S. McIntosh -- $tThe solar flare and CME induced as a collision of two opposite polarities on 1997 May 12 /$rL. Bharti, R. Jain, C. Joshi and S. Jaafferey -- $tInfluence of small-scale dynamics on large-scale solar activity /$rM. DeRosa -- $tQuiet sun unaffected by activity cycle /$rW. Livingston, D. Gray, L. Wallace and O. White -- $tThree dimensional numerical simulation of solar convection on MultiProcessors supercomputer systems /$rS. Ustyugov -- $tLarge-scale structures in distribution of coronal bright points /$rI. Sattarov, A. Pevtsov, N. Karachik and B. Sattarova -- $tComparison of the stream structure and coronal sources of the solar wind during the April 7 & May 12, 1997 halo CMEs /$rC. Arge, G. deToma and J. Luhmann -- $tMagnetically preferred solar longitudes : reality? /$rC. Henney and B. Durney -- $tHigh spectral resolution study of the He 10830 spectral region /$rO. Malanushenko, W. Livingston, H. Jones and V. Malanushenko -- $tActive longitudes in distribution of EIT bright points /$rI. Sattarov, A. Pevtsov, N. Karachik and B. Sattarova -- $tSunspot cycle 24 : smallest cycle in 100 years? /$rL. Svalgaard, E. Cliver and Y. Kamide -- $t22-year variations of the solar rotation /$rA. Tlatov and V. Makarov -- $tIndices of solar activity in minimum of sunspot cycles /$rA. Tlatov and V. Makarov -- $tThe observed MnI 539.47 nm spectral line in three sunspots of the NOAA 0431 complex active region /$rO. Vince and I. Vince.
530 $aAlso available via the World Wide Web.
651 0 $aSun$xActive regions$vCongresses.
700 1 $aSankarasubramanian, K.
700 1 $aPenn, M. J.$q(Matt J.)$0http://id.loc.gov/authorities/names/nr95047178
700 1 $aPevtsov, Alexei A.$0http://id.loc.gov/authorities/names/n99023736
830 0 $aAstronomical Society of the Pacific conference series ;$vv. 346.$0http://id.loc.gov/authorities/names/n86724091
856 41 $zOnline$uhttp://www.aspbooks.org/custom/publications/table%5Fof%5Fcontents/?book%5Fid=54
852 00 $boff,phy$hQB526.A37$iN37 2004g