Abstract: . . .  atmospheric parameters, chemical composition, degree of chromospheric activity, state of their evolution, mass, age, orbit eccentricity, ect. The thirteen stars that they felt future space based missions should consider for searching for Earth-like 7.3x107 W (13) This value agrees with the Radiometric Bode’s Law which states that Prad=εPisw (14) where Pisw is the solar wind power incident on the magnetosphere, and ε is a constant whose . . .
. . .  in Space Vol. 8, No. 7, March 1996, p. 9. APENDIX B: MAGNETIC FIELD STRENGTH IN CUSP AT 2RE θ=12º=.21 r=2RE RE=6x10^6m Br= 2Bo cos(θ) r 3 = 7.5x10-6T (B1) Bθ = Bo sin(θ) r 3 Farrell, W. M., et al., The radio search for extra-solar planets with LOFAR, Planetary and Space Science 52 (2004) 1469-1478. Lazio, W., et al., The Radiometric Bode’s Law and Extra-solar Planets, The Astrophysical Journal, 612:511-518, 2004 Sept. 1. Porto . . .
. . .  Mello, et al., Astrobiologically Interesting Stars within 10 parsecs of the Sun, Observatório Nacional, Rua Gen. José Cristino 77, Rio de Janeiro, 20921400 Brazil. Stevens, I. R., Magnetospheric Radio Emission from Extra-solar Giant Planets: The Role of the Host Stars, Mon. Not. R. Astron. Soc., Oct. 25, 2004. = 6x10-6T (B2) (B3) (B4) Bϕ =0T B= Bθ 2 + Br 2 = 9.6x10 -6T References Books Gehrels, T., Jupiter: Studies of the interior, . . .
. . .  Astrobiologically Interesting Stars within 10 parsecs of the Sun, Observatório Nacional, Rua Gen. José Cristino 77, Rio de Janeiro, 20921400 Brazil. Stevens, I. R., Magnetospheric Radio Emission from Extra-solar Giant Planets: The Role of the Host Stars, Mon. Not. R. Astron. Soc., Oct. 25, 2004. = 6x10-6T (B2) (B3) (B4) Bϕ =0T B= Bθ 2 + Br 2 = 9.6x10 -6T References Books Gehrels, T., Jupiter: Studies of the interior, atmosphere, . . .
. . .  altered field lines of the earth’s dipole represent the magnetosphere. This model does not represent the field of the magnetotail. See APPENDIX A: IMAGE DIPOLE MODEL EQUATIONS for the equations of the magnetosphere using the image dipole method in cartesian and spherical form. Some of the magnetic field lines that would connect in front on the day side of the earth are swept back and form the outer boundaries of the magnetotail. . . .
. . . For the UCLA Summer ’05 REU Program Searching for Extra-Solar Planets Using Non-Thermal Radio Continuum Emission Kimberly R. Trent Applied Physics, Yale University, New Haven, Connecticut 06520 Dr. Mike Jura Dept. of Physics and Astronomy, University of California at Los Angeles, Los Angeles, . . .
. . .  Sept. 1. Porto de Mello, et al., Astrobiologically Interesting Stars within 10 parsecs of the Sun, Observatório Nacional, Rua Gen. José Cristino 77, Rio de Janeiro, 20921400 Brazil. Stevens, I. R., Magnetospheric Radio Emission from Extra-solar Giant Planets: The Role of the Host Stars, Mon. Not. R. Astron. Soc., Oct. 25, 2004. = 6x10-6T (B2) (B3) (B4) Bϕ =0T B= Bθ 2 + Br 2 = 9.6x10 -6T References Books Gehrels, T., Jupiter: . . .
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