Log InRegister
Quick Links : The Mindat ManualThe Rock H. Currier Digital LibraryMindat Newsletter [Free Download]
Home PageAbout MindatThe Mindat ManualHistory of MindatCopyright StatusWho We AreContact UsAdvertise on Mindat
Donate to MindatCorporate SponsorshipSponsor a PageSponsored PagesMindat AdvertisersAdvertise on Mindat
Learning CenterWhat is a mineral?The most common minerals on earthInformation for EducatorsMindat ArticlesThe ElementsThe Rock H. Currier Digital LibraryGeologic Time
Minerals by PropertiesMinerals by ChemistryMineral Visual ExplorerAdvanced Locality SearchRandom MineralRandom LocalitySearch by minIDLocalities Near MeSearch ArticlesSearch GlossaryMore Search Options
Search For:
Mineral Name:
Locality Name:
Keyword(s):
 
The Mindat ManualAdd a New PhotoRate PhotosLocality Edit ReportCoordinate Completion ReportAdd Glossary Item
Mining CompaniesStatisticsUsersMineral MuseumsClubs & OrganizationsMineral Shows & EventsThe Mindat DirectoryDevice SettingsThe Mineral QuizTime Machine
Photo SearchPhoto GalleriesSearch by ColorPhoto Colour ExplorerNew Photos TodayNew Photos YesterdayMembers' Photo GalleriesPast Photo of the Day GalleryPhotography

Ng, C. S., Bhattacharjee, A., Munsi, D., Isenberg, P. A., Smith, C. W. (2010) Kolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja014377

Advanced
   -   Only viewable:
Reference TypeJournal (article/letter/editorial)
TitleKolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind
JournalJournal of Geophysical Research: Space Physics
AuthorsNg, C. S.Author
Bhattacharjee, A.Author
Munsi, D.Author
Isenberg, P. A.Author
Smith, C. W.Author
Year2010 (February)Volume115
PublisherAmerican Geophysical Union (AGU)
DOIdoi:10.1029/2009ja014377Search in ResearchGate
Generate Citation Formats
Mindat Ref. ID4591015Long-form Identifiermindat:1:5:4591015:5
GUID0
Full ReferenceNg, C. S., Bhattacharjee, A., Munsi, D., Isenberg, P. A., Smith, C. W. (2010) Kolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja014377
Plain TextNg, C. S., Bhattacharjee, A., Munsi, D., Isenberg, P. A., Smith, C. W. (2010) Kolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja014377
In(2010) Journal of Geophysical Research: Space Physics Vol. 115. American Geophysical Union (AGU)

See Also

These are possibly similar items as determined by title/reference text matching only.

Oughton, S., Matthaeus, W. H., Smith, C. W., Breech, B., Isenberg, P. A. (2011) Transport of solar wind fluctuations: A two-component model. Journal of Geophysical Research: Space Physics, 116. doi:10.1029/2010ja016365
Burke, W. J., Gentile, L. C., Hagan, M. P. (2010) Thermospheric heating by high-speed streams in the solar wind. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja014585
Bamert, K., Kallenbach, R., le Roux, J. A., Hilchenbach, M., Smith, C. W., Wurz, P. (2008) Evidence for Iroshnikov-Kraichnan-Type Turbulence in the Solar Wind Upstream of Interplanetary Traveling Shocks. The Astrophysical Journal, 675 (1). doi:10.1086/529491
Bhattacharjee, A., Ng, C. S., Ghosh, S., Goldstein, M. L. (1999) A comparative study of four-field and fully compressible magnetohydrodynamic turbulence in the solar wind. Journal of Geophysical Research: Space Physics, 104. 24835-24843 doi:10.1029/1999ja900327
Pulkkinen, T. I., Palmroth, M., Janhunen, P., Koskinen, H. E. J., McComas, D. J., Smith, C. W. (2010) Timing of changes in the solar wind energy input in relation to ionospheric response. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2010ja015764
Gray, P. C., Smith, C. W., Matthaeus, W. H., Otani, N. F. (1996) Heating of the solar wind by pickup ion driven Alfvén ion cyclotron instability. Geophysical Research Letters, 23 (2) 113-116 doi:10.1029/95gl03707
Henri, P., Califano, F., Briand, C., Mangeney, A. (2010) Vlasov-Poisson simulations of electrostatic parametric instability for localized Langmuir wave packets in the solar wind. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja014969
Breech, B., Matthaeus, W. H., Minnie, J., Bieber, J. W., Oughton, S., Smith, C. W., Isenberg, P. A. (2008) Turbulence transport throughout the heliosphere. Journal of Geophysical Research: Space Physics, 113. doi:10.1029/2007ja012711
Delamere, P. A., Bagenal, F. (2010) Solar wind interaction with Jupiter's magnetosphere. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2010ja015347
Isenberg, P. A., Chih, P. P., Fisk, L. A. (1985) The heating of the solar wind by the interstellar neutral gas. Journal of Geophysical Research, 90. 12040 doi:10.1029/ja090ia12p12040
Fry, C. D., Sun, W., Deehr, C. S., Dryer, M., Smith, Z., Akasofu, S.-I., Tokumaru, M., Kojima, M. (2001) Improvements to the HAF solar wind model for space weather predictions. Journal of Geophysical Research: Space Physics, 106. 20985-21001 doi:10.1029/2000ja000220
 
and/or  
Mindat.org® is an outreach project of the Hudson Institute of Mineralogy, a 501(c)(3) not-for-profit organization. Mindat® and mindat.org® are registered trademarks of the Hudson Institute of Mineralogy.
Copyright © mindat.org and the Hudson Institute of Mineralogy 1993-2026, except where stated. Most political location boundaries are © OpenStreetMap contributors. Mindat.org relies on the contributions of thousands of members and supporters. Founded in 2000 by Jolyon Ralph and Ida Chau.
To cite: Ralph, J., Von Bargen, D., Martynov, P., Zhang, J., Que, X., Prabhu, A., Morrison, S. M., Li, W., Chen, W., & Ma, X. (2025). Mindat.org: The open access mineralogy database to accelerate data-intensive geoscience research. American Mineralogist, 110(6), 833–844. doi:10.2138/am-2024-9486.
Privacy Policy - Terms & Conditions - Contact Us / DMCA issues - Report a bug/vulnerability Current server date and time: June 4, 2026 17:42:33
Go to top of page