1,721,276 research outputs found
P. Papini Stati Achilleis, rec. Aldo Marastoni
No full textDesmed R. P. Papini Stati Achilleis, rec. Aldo Marastoni. In: Scriptorium, Tome 31 n°1, 1977. pp. 170-171
Aldo Marastoni, P. Papini Statt Achilleis
No full textVerdière Raoul. Aldo Marastoni, P. Papini Statt Achilleis. In: L'antiquité classique, Tome 45, fasc. 1, 1976. p. 286
Aldo Marastoni, P. Papini Stati Silvae
No full textvan de Woestijne Paul. Aldo Marastoni, P. Papini Stati Silvae. In: L'antiquité classique, Tome 31, fasc. 1-2, 1962. pp. 365-366
P. Papini Stati, Achilleis, éd. A. Marastoni
No full textJ. A. P. Papini Stati, Achilleis, éd. A. Marastoni. In: Bulletin de l'Association Guillaume Budé, n°2, juin 1976. p. 201
P. Papini Stati Siluae, rec. Aldus Marastoni, editio stereotypa correctior.
No full textJ. A. P. Papini Stati Siluae, rec. Aldus Marastoni, editio stereotypa correctior.. In: Bulletin de l'Association Guillaume Budé, n°3, octobre 1972. p. 371
R. D. Williams, P. Papini Stati Thebaidos Liber Decimus
No full textVerdière Raoul. R. D. Williams, P. Papini Stati Thebaidos Liber Decimus. In: L'antiquité classique, Tome 42, fasc. 1, 1973. pp. 282-283
Paolo Venini, P. Papini Stati Thebaidos Liber XI. Introduction, texte, commentaire et traduction
No full textVerdière Raoul. Paolo Venini, P. Papini Stati Thebaidos Liber XI. Introduction, texte, commentaire et traduction. In: L'antiquité classique, Tome 41, fasc. 1, 1972. pp. 330-332
P. Papini Stati Siluae. Recensuit Aldus Marastoni (Bibliotheca Scriptorum Graecorum et Romanorum Teubneriana), 1961
No full textLe Bonniec Henri. P. Papini Stati Siluae. Recensuit Aldus Marastoni (Bibliotheca Scriptorum Graecorum et Romanorum Teubneriana), 1961. In: Revue des Études Anciennes. Tome 64, 1962, n°1-2. p. 209
An estimate of the secondary-proton spectrum at small atmospheric depths
No full textWe have calculated the energy spectrum of secondary protons produced in the atmosphere as a function of the atmospheric depth and zenith angles at a location with zero geomagnetic cut-off. In this calculation, we have included all relevant energy losses and production processes. It is shown that the protons produced from the target nuclei through recoil and evaporation processes dominate the spectrum below 350 MeV. These calculations have been carried out over an energy region from 20 MeV to 40 GeV and up to a depth of 40 g/cm2 of the atmosphere over a latitude with zero geomagnetic cut-off for both the periods of minimum and maximum solar modulation
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