Solar wind reflection from the lunar surface: The view from far and near

The Moon appears bright in the sky as a source of energetic neutral atoms (ENAs). These ENAs have recently been imaged over a broad energy range both from near the lunar surface, by India's Chandrayaan-1 mission (CH-1), and from a much more distant Earth orbit by NASA's Interstellar Boundary Explorer (IBEX) satellite. Both sets of observations have indicated that a relatively large fraction of the solar wind is reflected from the Moon as energetic neutral hydrogen. CH-1's angular resolution over different viewing angles of the lunar surface has enabled measurement of the emission as a function of angle. IBEX in contrast views not just a swath but a whole quadrant of the Moon as effectively a single pixel, as it subtends even at the closest approach no more than a few degrees on the sky. Here we use the scattering function measured by CH-1 to model global lunar ENA emission and combine these with IBEX observations. The deduced global reflection is modestly larger (by a factor of 1.25) when the angular scattering function is included. This provides a slightly updated IBEX estimate of AH=0.11±0.06 for the global neutralized albedo, which is ˜25% larger than the previous values of 0.09±0.05, based on an assumed uniform scattering distribution.

Proton entry into the near-lunar plasma wake for magnetic field aligned flow

We report the first observation of protons in the near-lunar (100-200 km from the surface) and deeper (near anti-subsolar point) plasma wake when the interplanetary magnetic field (IMF) and solar wind velocity (vsw) are parallel (aligned flow; angle between IMF and vsw≤10°). More than 98% of the observations during aligned flow condition showed the presence of protons in the wake. These observations are obtained by the Solar Wind Monitor sensor of the Sub-keV Atom Reflecting Analyser experiment on Chandrayaan-1. The observation cannot be explained by the conventional fluid models for aligned flow. Back tracing of the observed protons suggests that their source is the solar wind. The larger gyroradii of the wake protons compared to that of solar wind suggest that they were part of the tail of the solar wind velocity distribution function. Such protons could enter the wake due to their large gyroradii even when the flow is aligned to IMF. However, the wake boundary electric field may also play a role in the entry of the protons into the wake.

Establishing occupational and environmental health design requirements for Lunar and Mars settlements

In a study of Lunar and Mars settlement concepts, an analysis was made of fundamental design assumptions in five technical areas against a model list of occupational and environmental health concerns. The technical areas included the proposed science projects to be supported, habitat and construction issues, closed ecosystem issues, the "MMM" issues--mining, material-processing, and manufacturing, and the human elements of physiology, behavior and mission approach. Four major lessons were learned. First it is possible to relate public health concerns to complex technological development in a proactive design mode, which has the potential for long-term cost savings. Second, it became very apparent that prior to committing any nation or international group to spending the billions to start and complete a lunar settlement, over the next century, that a significantly different approach must be taken from those previously proposed, to solve the closed ecosystem and "MMM" problems. Third, it also appears that the health concerns and technology issues to be addressed for human exploration into space are fundamentally those to be solved for human habitation of the earth (as a closed ecosystem) in the 21st century. Finally, it is proposed that ecosystem design modeling must develop new tools, based on probabilistic models as a step up from closed circuit models. ^

On vertical electric fields at lunar magnetic anomalies

We study the interaction between a magnetic dipole mimicking the Gerasimovich magnetic anomaly on the lunar surface and the solar wind in a self-consistent 3-D quasi-neutral hybrid simulation where ions are modeled as particles and electrons as a charge-neutralizing fluid. Especially, we consider the origin of the recently observed electric potentials at lunar magnetic anomalies. An antimoonward Hall electric field forms in our simulation resulting in a potential difference of <300V on the lunar surface, in which the value is similar to observations. Since the hybrid model assumes charge neutrality, our results suggest that the electric potentials at lunar magnetic anomalies can be formed by decoupling of ion and electron motion even without charge separation.

First direct observation of sputtered lunar oxygen

We present the first direct measurement of neutral oxygen in the lunar exosphere, detected by the Chandrayaan-1 Energetic Neutral Analyzer (CENA). With the lunar surface consisting of about 60% of oxygen in number, the neutral oxygen detected in CENA's energy range (11 eV−3.3 keV) is attributed to have originated from the lunar surface, where it was released through solar wind ion sputtering. Fitting of CENA's mass spectra with calibration spectra from ground and in-flight data resulted in the detection of a robust oxygen signal, with a flux of 0.2 to 0.4 times the flux of backscattered hydrogen, depending on the solar wind helium content and particle velocity. For the two solar wind types observed, we derive subsolar surface oxygen atom densities of N0= (1.1 ± 0.3) · 107m−3 and (1.4 ± 0.4) · 107m−3, respectively, which agree well with earlier model predictions and measured upper limits. From these surface densities, we derive column densities of NC= (1.5 ± 0.5) · 1013 m−2and (1.6 ± 0.5) · 1013 m−2. In addition, we identified for the first time a helium component. This helium is attributed to backscattering of solar wind helium (alpha particles) from the lunar surface as neutral energetic helium atoms, which has also been observed for the first time. This identification is supported by the characteristic energy of the measured helium atoms, which is roughly 4 times the energy of reflected solar wind hydrogen, and the correlation with solar wind helium content.

Chandrayaan-1 observations of backscattered solar wind protons from the lunar regolith: Dependence on the solar wind speed

We study the backscattering of solar wind protons from the lunar regolith using the Solar Wind Monitor of the Sub-keV Atom Reflecting Analyzer on Chandrayaan-1. Our study focuses on the component of the backscattered particles that leaves the regolith with a positive charge. We find that the fraction of the incident solar wind protons that backscatter as protons, i.e., the proton-backscattering efficiency, has an exponential dependence on the solar wind speed that varies from ~0.01% to ~1% for solar wind speeds of 250 km/s to 550 km/s. We also study the speed distribution of the backscattered protons in the fast (~550 km/s) solar wind case and find both a peak speed at ~80% of the solar wind speed and a spread of ~85 km/s. The observed flux variations and speed distribution of the backscattered protons can be explained by a speed-dependent charge state of the backscattered particles.

New fully kinetic model for the study of electric potential, plasma, and dust above lunar landscapes

We have developed a new fully kinetic electrostatic simulation, HYBes, to study how the lunar landscape affects the electric potential and plasma distributions near the surface and the properties of lifted dust. The model embodies new techniques that can be used in various types of physical environments and situations. We demonstrate the applicability of the new model in a situation involving three charged particle species, which are solar wind electrons and protons, and lunar photoelectrons. Properties of dust are studied with test particle simulations by using the electric fields derived from the HYBes model. Simulations show the high importance of the plasma and the electric potential near the surface. For comparison, the electric potential gradients near the landscapes with feature sizes of the order of the Debye length are much larger than those near a flat surface at different solar zenith angles. Furthermore, dust test particle simulations indicate that the landscape relief influences the dust location over the surface. The study suggests that the local landscape has to be taken into account when the distributions of plasma and dust above lunar surface are studied. The HYBes model can be applied not only at the Moon but also on a wide range of airless planetary objects such as Mercury, other planetary moons, asteroids, and nonactive comets.

Na 1 Nachlass Max Horkheimer, 652 - Vorlesungen: "National Socialism", "Autoritarian doctrines and modern European institutions", "Eclipse of Reason" (p. IX 35a.1-2-IX 36.1-5b)

"National Socialism": 1. Ankündigung einer Vorlesungsreihe November/Dezember 1941 von: Herbert Marcuse, A.R.L. Gurland, Franz Neumann, Otto Kirchheimer, Frederick Pollock. a) als Typoskript verfielfältigt, 1 Blatt, b) Typoskript, 1 Blatt; 2. Antwortbrief auf Einladungen zur Vorlesungsreihe, von Neilson, William A.; Packelis, Alexander H.; Michael, Jerome; McClung Lee, Alfred; Youtz, R.P.; Ginsburg, Isidor; Ganey, G.; Nunhauer, Arthur. 8 Blätter; "Autoritarian doctrines and modern European institutions" (1924): 1. Vorlesungs-Ankündigung Typoskript, 2 Blatt; 2. Ankündigungen der Vorlesungen von Neumann, Franz L.: "Stratification and Dominance in Germany"; "Bureaucracy as a Social and Political Institution", Typoskript, 2 Blatt; 3. Evans, Austin P.: 1 Brief (Abschrift) an Frederick Pollock, New York, 26.2.1924; "Eclipse of Reason", Fünf Vorlesungen 1943/44:; 1. I. Lecture. a) Typoskript mit eigenhändigen Korrekturen, 38 Blatt b) Typoskript, 29 Blatt c) Typoskript mit eigenhändigen und handschriftlichen Korrekturen, 31 Blatt d) Teilstück, Typoskript mit eigenhändigen Korrekturen, 2 Blatt e) Entwürfe, Typoskript mit eigenhändigen Korrekturen, 6 Blatt; 2. II. Lecture. a) Typoskript mit eigenhändigen Korrekturen, 27 Blatt, b) Typoskript mit handschriftlichen Korrekturen, 37 Blatt; 3. III. Lecture. Typoskript mit eigenhändigen Korrekturen, 27 Blatt; 4. IV. Lecture. Typoskript mit eigenhändigen Korrekturen, 23 Blatt; 5. V. Lecture. a) Typoskript mit eigenhändigen Korrekturen, 25 Blatt, b) Teilstücke, Typoskript mit eigenhändigen und handschriftlichen Korrekturen, 3 Blatt;

Na 1 Nachlass Max Horkheimer, 653 - Vorlesungen: "Eclipse of Reason"; "Society and Reason" (p. IX 36.6-12)

6. Vorlesungen 1. - 5. mit dem Titel "Society and Reason". a) Typoskript mit handschriftlichen Randbemerkungen von Theodor W. Adorno, 139 Blatt b) Typoskript, 139 Blatt; 7. Teilstück, Typoskript mit eigenhändigen Korrekturen, 1 Blatt; 8. Eigenhändige Notizen, 4 Blatt; 9. Stichworte zu den Vorlesungen I-III. Typoskript mit eigenhändigen Ergänzungen, 2 Blatt a) Einladungskarte zur Vorlesungsreihe "Society and Reason". Als Typoskript vervielfältigt, 1 Blatt b) Gliederung. Typoskript, 1 Blatt; 10. "Über Probleme des wissenschaftlichen Stils". Reaktion auf ein Schriftstück (aus einem Brief an Friedrich Pollock). a) Typoskript, datiert: 28.11.1943, 3 Blatt b) Max Horkheimer: 1 Brief an Friedrich Pollock, ohne Ort, 28.11.1943, 5 Blatt; 11. Columbia University, New York: 1 Brief (Abschrift) an Max Horkheimer, New York, 5.3.1943, und Stichworte zu den Vorlesungen, 2 Blatt; 12. Zeitungsausschnitt, 1 Blatt.;

Current measurements below the ice in Eclipse Sound

Velocity and direction of the current under the sea ice of the EcIipse Sound between Baffin lsland and Bylot Island were measured with specially developed devices and registered on a recorder. During the period of registration (May-June 1972) an easterly current of 5-7 cm/s superimposed by tidal and local influences (max. 12 cm/s) was found. In addition , measurements of friction between steelcone surfaces und corresponding conical ice bores are reported on. The plotted results show the influence of ice-temperature, surface quality and in some cases the influence of time.

Respuestas antiguas y contemporáneas ante el anuncio de catástrofes : Píndaro, el Peán 9 ante el eclipse de sol y los pronósticos del cambio climático

El presente artículo investiga algunas respuestas de la sociedad ante el pronóstico de calamidades comunitarias, estableciendo una comparación entre la respuesta de una comunidad antigua y algunas respuestas de la sociedad globalizada del siglo XXI ante los pronósticos científicos concernientes al cambio climático. En el campo disciplinar de la filología, se propone una lectura más compleja del Peán 9 de Píndaro (fr. 52k Maehler = A1 Rutherford), que busca dar cuenta del fenómeno del eclipse de sol, descrito por el poeta como un signo de catástrofes comunitarias, en el marco de los posibles conocimientos astronómicos de la época, y en la red de significados implícita en las formas de pensamiento simbólico propias de la Grecia arcaica. Tanto las actitudes antiguas como las actuales ante el anuncio de calamidades comunitarias se consideran desde una perspectiva antropológica apoyada en la investigación moderna sobre mitología.