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Shibata, Kazunari, Suematsu, Yoshinori (1982) Why are spicules absent over plages and long under coronal holes?. Solar Physics, 78 (2). 333-345 doi:10.1007/bf00151612

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Reference TypeJournal (article/letter/editorial)
TitleWhy are spicules absent over plages and long under coronal holes?
JournalSolar Physics
AuthorsShibata, KazunariAuthor
Suematsu, YoshinoriAuthor
Year1982 (June)Volume78
Issue2
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/bf00151612Search in ResearchGate
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Mindat Ref. ID8917262Long-form Identifiermindat:1:5:8917262:5
GUID0
Full ReferenceShibata, Kazunari, Suematsu, Yoshinori (1982) Why are spicules absent over plages and long under coronal holes?. Solar Physics, 78 (2). 333-345 doi:10.1007/bf00151612
Plain TextShibata, Kazunari, Suematsu, Yoshinori (1982) Why are spicules absent over plages and long under coronal holes?. Solar Physics, 78 (2). 333-345 doi:10.1007/bf00151612
In(1982, June) Solar Physics Vol. 78 (2) Springer Science and Business Media LLC

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Suematsu, Yoshinori, Shibata, Kazunari, Nishikawa, Takara, Kitai, Reizaburo (1982) Numerical hydrodynamics of the jet phenomena in the solar atmosphere. Solar Physics, 75 (1). 99-118 doi:10.1007/bf00153464
Shibata, Kazunari, Nishikawa, Takara, Kitai, Reizaburo, Suematsu, Yoshinori (1982) Numerical hydrodynamics of the jet phenomena in the solar atmosphere. Solar Physics, 77 (1). 121-151 doi:10.1007/bf00156100
Kudoh, Takahiro, Shibata, Kazunari (1999) Alfven Wave Model of Spicules and Coronal Heating. The Astrophysical Journal, 514 (1). 493-505 doi:10.1086/306930
Sterling, Alphonse C., Mariska, John T., Shibata, Kazunari, Suematsu, Yoshinori (1991) Numerical simulations of microflare evolution in the solar transition region and corona. The Astrophysical Journal, 381. 313pp. doi:10.1086/170653
Parker, Gary D. (1986) Lifetime, age, and rotation of coronal magnetic fields. Solar Physics, 104 (2). 333-345 doi:10.1007/bf00159086
Baker, Kile B., Papagiannis, Michael D. (1982) Correlation of high latitude coronal holes with solar wind streams far above or below the ecliptic. Solar Physics, 78 (2). 365-372 doi:10.1007/bf00151616
Shibata, Kazunari (1982) Two types of jets and origin of macrospicules. Solar Physics, 81 (1). 9-17 doi:10.1007/bf00151974
Simon, PaulA. (1979) Polar coronal holes and solar cycles. Solar Physics, 63 (2). doi:10.1007/bf00174544
Yeh, Tyan (1982) A magnetohydrodynamic theory of coronal loop transients. Solar Physics, 78 (2). 287-316 doi:10.1007/bf00151610
Alissandrakis, Constantine E. (1973) A spectroscopic study of solar spicules in H?, H? and K. Solar Physics, 32 (2). 345-359 doi:10.1007/bf00154947
Beck, C., Rezaei, R., Puschmann, K. G., Fabbian, D. (2016) Spectroscopy at the Solar Limb: II. Are Spicules Heated to Coronal Temperatures?. Solar Physics, 291 (8). 2281-2328 doi:10.1007/s11207-016-0964-4
 
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