{"id":14,"date":"2022-05-02T20:13:18","date_gmt":"2022-05-02T20:13:18","guid":{"rendered":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/?page_id=14"},"modified":"2024-04-29T07:47:26","modified_gmt":"2024-04-29T07:47:26","slug":"meetings","status":"publish","type":"page","link":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/meetings\/","title":{"rendered":"Meetings"},"content":{"rendered":"<p>List of presentations stimulating the discussion of the team during the in-person meetings in Bern.<\/p>\n<p><strong>1st in-person meeting<\/strong>: June 20-24, 2022, ISSI Bern, Switzerland<\/p>\n<ul>\n<li><strong>J. Heerikhuisen<\/strong>, Structure of the heliosphere as a function of a variety of physical processes<\/li>\n<li><strong>M. Kornbleuth<\/strong>, A comparison of the croissant-like and comet-like heliotail configuration resulting from different MHD models<\/li>\n<li><strong>M. Kornbleuth<\/strong>, Effects of varying solar wind conditions in a steady state heliosphere<\/li>\n<li><strong>P. Swaczyna<\/strong>, Interstellar parameters derived from ISN He observations by IBEX<\/li>\n<li><strong>M. Opher<\/strong>, Discussion on the assumption on BU model and future development of the SHIELD model<\/li>\n<li><strong>A. Galli<\/strong>, One solar cycle of heliosphere obervations with IBEX: Energetic neutral hydrogen atoms observed with IBEX-Lo from 10 eV to 2 keV<\/li>\n<li><strong>K. Dialynas<\/strong>, On the properties of 0.11 keV to 344 MeV ion spectra in the inner heliosheath using regularizerd kappa distribution<\/li>\n<li><strong>M. Kornbleuth<\/strong>, A comparison of the croissant-like and comet-like heliotail configuration resulting from MHD models in modeled ENA maps<\/li>\n<li><strong>K. Dialynas<\/strong>, Gkioulidou et al. paper: differences between the 0.5-55 keV ENA measured spectra and corresponding spectra from models<\/li>\n<li><strong>D. Koutroumpa<\/strong>, Inversion of SWAN Ly-alpha maps &#8211; deriving calibrated total ionization rates for ISN H atoms<\/li>\n<li><strong>M. Bzowski<\/strong>, WawHelioGlow: the Warsaw model of the heliospheric backscatter glow and comparison with selected SWAN observations<\/li>\n<li><strong>P. Swaczyna<\/strong>, Elastic and charge exchange collisions &#8211; the angular scattering of ISN atoms<\/li>\n<li><strong>M. Bzowski<\/strong>, WawHelIon &#8211; the Warsaw heliospheric ionization model, with special emphasis on the evolution of the solar wind structure<\/li>\n<li><strong>H.-R. <\/strong><strong>M\u00fcller<\/strong>, Absorption of stellar Lyman-alpha by the heliospheric hydrogen wall<\/li>\n<li><strong>I. Kowalska-Leszczy\u0144ska<\/strong>, Absorption of the Lyman-alpha profile line<\/li>\n<li><strong>F. Rahamanifard<\/strong>, Effects of rafiation pressure on ISN H observations by IBEX. Simulating ISN H fluxes to be observed inside the heliosphere<\/li>\n<li><strong>A. Galli<\/strong>, Summary of the findings from the Galli et al. 2019 paper ISN H IBEX-Lo observation paper<\/li>\n<li><strong>P. Swaczyna<\/strong>, Bulk flow and distribution of ISN He at 100 au<\/li>\n<li><strong>H.-R. <\/strong><strong>M\u00fcller<\/strong>, Trajectory methods for neutral velocity distribution functions in the heliosphere<strong><br \/>\n<\/strong><\/li>\n<li><strong>M. Bzowski<\/strong>, Time- and solar distance evolution of ISN H in the heliosphere and PUI fluxes based on WTPM, WawHelIon and WawHelioUV<\/li>\n<li><strong>P. Swaczyna<\/strong>, H PUI observed on SWAP\/New Horizons<\/li>\n<\/ul>\n<p><strong>2nd in-person meeting<\/strong>: October 9-13, 2023, ISSI Bern, Switzerland<\/p>\n<ul>\n<li><strong>M. Kornbleuth<\/strong>, Inferring the Interstellar Magnetic Field Direction from Energetic Neutral Atom Observations of the Heliotail<\/li>\n<li><strong>J. Heerikhuisen<\/strong>, Hydrogen and Helium in the Solar Wind<\/li>\n<li><strong>F. Fraternale<\/strong>, Global modeling of the SW-LISM interaction with kinetic neutral atoms: role of electrons, helium ions and effects on the neutrals distributions<\/li>\n<li><strong>M. Kornbleuth<\/strong>, Probing the Length of the Heliospheric Tail with ENAs from 0.52-80 keV<\/li>\n<li><strong>L. Dyke<\/strong>, Using trajectory methods to examine velocity distribution functions of primary interstellar neutral hydrogen in a time-dependent force environment<\/li>\n<li><strong>H.-R. <\/strong><strong>M\u00fcller<\/strong>, Neutral hydrogen velocity distribution functions at a r=100 au reference distance, obtained by trajectory methods<\/li>\n<li><strong>P. Swaczyna<\/strong>, Discussion on the ISN H filtration in the various models vs. NH observations<\/li>\n<li><strong>Chika Onobugo<\/strong> (M. Opher\u2019s student), Effect of Turbulent Heliospheric Tail on capturing Heliopause<\/li>\n<li><strong>Erick Powell<\/strong> (M. Opher\u2019s student), Constraints on BISM from Lyman-alpha<\/li>\n<li><strong>D. Koutroumpa<\/strong>, Heliospheric interface diagnostics with high-resolution X-ray spectroscopy using micro-calorimeters<\/li>\n<li><strong>M. Bzowski<\/strong>, The Direction of the Flow of Interstellar Neutral H Based on Photometric Observations from SOHO\/SWAN<\/li>\n<li><strong>I. Kowalska-Leszczy\u0144ska<\/strong>, Response of the Ly-alpha glow on time-evolution of the ionization and solar Ly-alpha line intensity.<\/li>\n<li><strong>A. Galli<\/strong>, New general paper incl. data release of all model-free ISN H maps for all years from 2009-2023<\/li>\n<li><strong>F. Rahmanifard<\/strong>, The Effect of Angular Scattering Imposed by Charge Exchange and Elastic Collisions on Interstellar Neutral Hydrogen Atoms<\/li>\n<li><strong> P. Swaczyna<\/strong>, Updated interstellar conditions from ISN helium observations<\/li>\n<li><strong>H.-R. <\/strong><strong>M\u00fcller<\/strong>, Update about absorption of stellar Ly-alpha radiation in the hydrogen wall (TBC)<\/li>\n<li><strong>K. Dialynas<\/strong>, Anisotropies of 40-139 keV ions beyond the TS and in the VLISM: Implications for ion spectra beyond the HP<\/li>\n<li><strong>F. Rahmanifard<\/strong>, Discussion of IBEX-Lo response to ISN H<\/li>\n<li><strong>A. Galli<\/strong>, The anomalously low ISN H energy measured with IBEX-Lo<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>List of presentations stimulating the discussion of the team during the in-person meetings in Bern. 1st in-person meeting: June 20-24, 2022, ISSI Bern, Switzerland J. Heerikhuisen, Structure of the heliosphere as a function of a variety of physical processes M. Kornbleuth, A comparison of the croissant-like and comet-like heliotail configuration resulting from different MHD models [&hellip;]<\/p>\n","protected":false},"author":38,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-14","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/pages\/14","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/users\/38"}],"replies":[{"embeddable":true,"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/comments?post=14"}],"version-history":[{"count":6,"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/pages\/14\/revisions"}],"predecessor-version":[{"id":35,"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/pages\/14\/revisions\/35"}],"wp:attachment":[{"href":"https:\/\/teams.issibern.ch\/interstellarneutralhydrogen\/wp-json\/wp\/v2\/media?parent=14"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}