Publikationen von Hardi Peter

Shapiro, A.; Peter, H.; Solanki, S. K.: The Sun's Atmosphere. In: The Sun as a Guide to Stellar Physics, S. 59 - 85 (Hg. Engvold, O.; Vial, .-C.; Skumanich, A.). Elsevier, Amsterdam (2019)

Ruan, W.; He, J.; Zhang, L.; Vocks, C.; Marsch, E.; Tu, C.; Peter, H.; Wang, L.: Synthetic Spectral Analysis of a Kinetic Model for Slow-Magnetosonic Waves in Solar Corona. In: Proceedings of the 14th International Solar Wind Conference (Hg. Wang, L.; Bruno, R.; Moebius, E.; Zank, G.). American Institute of Physics, Melville, NY, USA (2016)

Yang, L.; Zhang, L.; He, J.; Peter, H.; Tu, C.; Wang, L.; Feng, X.: Excitation Of Magnetohydrodynamic Waves By Plasmoids Ejection In The Solar Corona. In: Proceedings of the 14th International Solar Wind Conference (Hg. Wang, L.; Bruno, R.; Moebius, E.; Zank, G.). American Institute of Physics, Melville, NY, USA (2016)

Bingert, S.; Peter, H.: Nanoflare Heating in the Solar Corona. In: High Performance Computing in Science and Engineering 14, S. 113 - 120 (Hg. Nagel, W. E.; Kröner, D. H.; Resch, M. M.). Springer International Publishing, Switzerland (2015)

van Driel-Gesztelyi, L.; Schrijver, C. J.; Klimchuk, J. A.; Charbonneau, P.; Fletcher, L.; Hasan, S. S.; Hudson, H. S.; Kusano, K.; Mandrini, C. H.; Peter, H. et al.; Vrnak, B.; Yan, Y.: Commission 10: Solar Activity. In: Transactions IAU, S. 69 - 80 (Hg. Corbett, I.). (2012)

Brkovic, A.; Peter, H.; Solanki, S. K.: Relative brightness variability vs. averaged Doppler shift in the quiet Sun. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', S. 281 - 282 (Hg. Wilson, A.). ESA Publ. Div., Noordwijk (2002)

Peter, H.; Marsch, E.: Ionization layer of hydrogen in the solar chromosphere and the solar wind mass flux. In: Proc. Fifth SOHO Workshop ``The Corona and Solar Wind Near Minimum Activity'', Oslo, S. 591 - 594 (Hg. Wilson, A.). ESA Publ. Div., Noordwijk (1997)

Chitta, L. P.; Peter, H.; Solanki, S.: Coronal loop footpoints threaded with small-scale mixed polarity surface magnetic fields. SOLARNET IV: The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)

Cilla, A. A.; Chitta, L. P.; Peter, H.: Rotational motion in transition region loops. 8th Coronal Loops Workshop: many facets of magnetically closed corona, Palermo, Italy (2017)

Cilla, A. A.; Chitta, L. P.; Peter, H.: Signs of helical transition region loops embedded in filament channels. Rocks \& Stars II, Göttingen, Germany (2017)

Chitta, L. P.; Peter, H.; Young, P. R.: Chromospheric response to prolonged small-scale reconnections. IRIS-6: The Chromosphere, Stockholm, Sweden (2016)

Chen, F.; Peter, H.: Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. 2nd International Sino-German Symposium of Solar Physics: Multi Waveband Observations and Modeling of Solar Activity, Bad Honnef, Germany (2015)

Chitta, L. P.; Peter, H.; Young, P. R.: A closer look at the footpoints of coronal loops rooted in a sunspot umbra. Hinode 9 Science Meeting, Belfast, Ireland (2015)

Chen, F.; Peter, H.; Bingert, S.: Magnetic Field Lines and Coronal Loops A Difficult Relation. Living With a Star / Iris / Hinode Meeting, Portland, USA (2014)

Chen, F.; Peter, H.; Bingert, S.; Cheung, M. C. M.: Magnetic field lines and coronal loops. 14th European Solar Physics Meeting, Dublin, Ireland (2014)

Warnecke, J.; Peter, H.: Magnetic field lines in 3D MHD models of the solar corona. Max-Planck/Princeton Center for Plasma Physics, General Meeting, Berlin, Germany (2014)

Cilla, A. A.; Chitta, L. P.; Peter, H.: Signs of helical transition region loops embedded in filament channels. European Solar Physics Meeting, Budapest, Hungary (2017)

Fludra, A.; Haberreiter, M.; Peter, H.; Vial, J.-C.; Harrison, R.; Parenti, S.; Innes, D.; Schmutz, W.; Buchlin, E.; Chamberlin, P. et al.; Curdt, W.; coauthors, 2.: The SPICE Spectral Imager on Solar Orbiter: Linking the Sun to the Heliosphere. COSPAR-41, Istanbul, Turkey (2016)

Giunta, A.; Haberreiter, M.; Peter, H.; Vial, J.-C.; Harrison, R.; Parenti, S.; Innes, D.; Schmutz, W.; Buchlin, E.; Chamberlin, P. et al.; Curdt, W.; others: Solar abundances with the SPICE spectral imager on Solar Orbite. COSPAR-41, Istanbul, Turkey (2016)

Chen, F.; Peter, H.: Using coronal seismology to estimate the magnetic field strength in a realistic coronal model. Hinode 9 Science Meeting, Belfast, Ireland (2015)