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EDELGASE ALS VISITENKARTE. (LES GAZ RARES COMME CARTES DE VISITE).FAHR H.1970; KOSMOS-BIBLIOTHEK.-DTSCH; DEU; 1970(3), VOL. 66, NUM. 0003, P. 77 A 78Miscellaneous

Revisiting the theory of the evolution of pick-up ion distributions : magnetic or adiabatic cooling?FAHR, H. J.Annales geophysicae (1988). 2007, Vol 25, Num 12, pp 2649-2659, issn 0992-7689, 11 p.Article

COMPARISON OF GUINEA PIG SENSITIZATION METHODS.FAHR H; NOSTER U; SCHULZ KH et al.1976; CONTACT. DERMAT.; DENM.; DA. 1976; VOL. 2; NO 6; PP. 335-339; BIBL. 7 REF.Article

Solar wind heating by an embedded quasi-isothermal pick-up ion fluidFAHR, H. J.Annales geophysicae (1988). 2002, Vol 20, Num 10, pp 1509-1518, issn 0992-7689, 10 p.Article

Local interstellar oxygen in the heliosphere : its analytic representation and observational consequencesFAHR, H. J.Astronomy and astrophysics (Berlin. Print). 1991, Vol 241, Num 1, pp 251-259, issn 0004-6361, 9 p.Article

Is the heliospheric interface submagnetosonic? Consequences for the LISM presence in the heliosphereFAHR, H. J.Advances in space research. 1986, Vol 6, Num 2, pp 13-25, issn 0273-1177Conference Paper

The Maxwellian alternative to the dark matter problem in galaxiesFAHR, H. J.Astronomy and astrophysics (Berlin. Print). 1990, Vol 236, Num 1, pp 86-94, issn 0004-6361, 9 p.Article

Am Anfang war die Sonne blau = A l'origine le soleil était bleuFAHR, H. J.1984, Vol 21, Num 2, pp 76-82, issn 0006-2375Article

A SEARCH FOR INTERPLANETARY HE II, 304-A EMISSIONPARESCE F; FAHR H; LAY G et al.1981; J. GEOPHYS. RES.; ISSN 0022-1406; USA; DA. 1981; VOL. 86; NO A12; PP. 10038-10048; BIBL. 45 REF.Article

Pick-up ion transport under conservation of particle invariants: how important are velocity diffusion and cooling processes?FAHR, H. J; FICHTNER, H.Astronomy and astrophysics (Berlin. Print). 2011, Vol 533, issn 0004-6361, A92.1-A92.9, 2Article

A kinetic description of the dissipative quasi-parallel solar wind termination shockVERSCHAREN, D; FAHR, H.-J.Astronomy and astrophysics (Berlin. Print). 2008, Vol 487, Num 2, pp 723-729, issn 0004-6361, 7 p.Article

Solar cycle induced variations of the outer heliospheric structuresSCHERER, K; FAHR, H. J.Geophysical research letters. 2003, Vol 30, Num 2, pp 17.1-17.4, issn 0094-8276Article

The influence of electron impact ionization on the distribution of interstellar helium in the inner heliosphere; possible consequences for determination of interstellar helium parametersRUCINSKI, D; FAHR, H. J.Astronomy and astrophysics (Berlin. Print). 1989, Vol 224, Num 1-2, pp 290-298, issn 0004-6361Article

Heliopause imaging in EUV : Oxygen O+ ion 83.4-nm resonance line emissionGRUNTMAN, M; FAHR, H. J.Journal of geophysical research. 2000, Vol 105, Num A3, pp 5189-5200, issn 0148-0227Article

Photon stigmata from the recombination phase superimposed on the cosmological background radiationFAHR, H. J; LOCH, R.Astronomy and astrophysics (Berlin. Print). 1991, Vol 246, Num 1, pp 1-9, issn 0004-6361, 9 p.Article

Physical reasons and consequences of a three-dimensionally structured heliosphereFAHR, H.-J; FICHTNER, H.Space science reviews. 1991, Vol 58, Num 3-4, pp 193-258, issn 0038-6308Article

Fluctuations in the heliospheric hydrogen distribution induced by generalized and time-dependent interstellar boundary conditionsSCHERER, K; FAHR, H. J.Planetary and space science. 1990, Vol 38, Num 12, pp 1487-1493, issn 0032-0633, 7 p.Article

Plasma expansion from diverging magnetic field configurations: the plasma-magnetic field interactionFICHTNER, H; FAHR, H. J.Planetary and space science. 1989, Vol 37, Num 8, pp 987-999, issn 0032-0633Article

Radiation belt particles and OII emissions determined as contaminations of geocoronal helium airglow observationsFAHR, H. J; LAY, G.Journal of geophysics. 1984, Vol 54, Num 3, pp 219-229, issn 0340-062XArticle

Stationary plasma-field equilibrium states in astropause boundary layers. I: General theoryFAHR, H. J; NEUTSCH, W.Monthly Notices of the Royal Astronomical Society. 1983, Vol 205, Num 2, pp 839-857, issn 0035-8711Article

Upstream ions converting into downstream pick-up ions: the effect of shock-decelerated frozen-in fieldsFAHR, H.-J; SIEWERT, M.Astronomy and astrophysics (Berlin. Print). 2010, Vol 512, issn 0004-6361, 512A64.1-512A64.6Article

Kinetic study of the ion passage over the solar wind MHD termination shockFAHR, H.-J; SIEWERT, M.Astronomy and astrophysics (Berlin. Print). 2006, Vol 458, Num 1, pp 13-20, issn 0004-6361, 8 p.Article

Nonthermal ions of interstellar origin at different solar wind conditionsRUCINSKI, D; FAHR, H. J.Annales geophysicae (1988). 1991, Vol 9, Num 2, pp 102-110, issn 0992-7689, 9 p.Article

The step feature of suprathermal ion distributions: a discriminator between acceleration processes?FAHR, H. J; FICHTNER, H.Annales geophysicae (1988). 2012, Vol 30, Num 9, pp 1315-1319, issn 0992-7689, 5 p.Article

Spatial variation of the pickup-proton-injection rate into the ACR regime at the 3D-heliospheric termination shockSCHERER, K; FAHR, H.-J.Astronomy and astrophysics (Berlin. Print). 2009, Vol 495, Num 2, pp 631-638, issn 0004-6361, 8 p.Article

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