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Biomedical subjects

M J Wolff

Publications and source records attributed to M J Wolff.

12 recordsLinked to original sources
PubMed2005

Solar eclipses of Phobos and Deimos observed from the surface of Mars.

The small martian satellites Phobos and Deimos orbit in synchronous rotation with inclinations of only 0.01 degrees and 0.92 degrees , respectively, relative to the planet's equatorial plane. Thus, an observer at near-equatorial latitudes on Mars could occasionally observe solar eclipses by these satellites (see ref. 1, for example). Because the apparent angular diameter of the satellites is much smaller than that of the Sun, however, such events are more appropriately referred to as transits. Transit data can be used for correcting and refining the orbital ephemerides of the moons. For example, Phobos is known to exhibit a secular acceleration that is caused by tidal dissipation within Mars. Long-term, accurate measurements are needed to refine the magnitude and origin of this dissipation within the martian interior as well as to refine the predicted orbital evolution of both satellites. Here we present observations of six transits of Phobos and Deimos across the solar disk from cameras on Mars aboard the Mars Exploration Rovers Spirit and Opportunity. These are the first direct imaging observations of satellites transiting the Sun from the surface of another planet.

Journal Article↗
PubMed2004

Atmospheric imaging results from the Mars exploration rovers: Spirit and Opportunity.

A visible atmospheric optical depth of 0.9 was measured by the Spirit rover at Gusev crater and by the Opportunity rover at Meridiani Planum. Optical depth decreased by about 0.6 to 0.7% per sol through both 90-sol primary missions. The vertical distribution of atmospheric dust at Gusev crater was consistent with uniform mixing, with a measured scale height of 11.56 +/- 0.62 kilometers. The dust's cross section weighted mean radius was 1.47 +/- 0.21 micrometers (mm) at Gusev and 1.52 +/- 0.18 mm at Meridiani. Comparison of visible optical depths with 9-mm optical depths shows a visible-to-infrared optical depth ratio of 2.0 +/- 0.2 for comparison with previous monitoring of infrared optical depths.

Algorithms↗
PubMed2004

Mineralogy at Meridiani Planum from the Mini-TES Experiment on the Opportunity Rover.

The Miniature Thermal Emission Spectrometer (Mini-TES) on Opportunity investigated the mineral abundances and compositions of outcrops, rocks, and soils at Meridiani Planum. Coarse crystalline hematite and olivine-rich basaltic sands were observed as predicted from orbital TES spectroscopy. Outcrops of aqueous origin are composed of 15 to 35% by volume magnesium and calcium sulfates [a high-silica component modeled as a combination of glass, feldspar, and sheet silicates (approximately 20 to 30%)], and hematite; only minor jarosite is identified in Mini-TES spectra. Mini-TES spectra show only a hematite signature in the millimeter-sized spherules. Basaltic materials have more plagioclase than pyroxene, contain olivine, and are similar in inferred mineral composition to basalt mapped from orbit. Bounce rock is dominated by clinopyroxene and is close in inferred mineral composition to the basaltic martian meteorites. Bright wind streak material matches global dust. Waterlain rocks covered by unaltered basaltic sands suggest a change from an aqueous environment to one dominated by physical weathering.

Calcium Sulfate↗
PubMed2004

Pancam multispectral imaging results from the Opportunity Rover at Meridiani Planum.

Panoramic Camera (Pancam) images from Meridiani Planum reveal a low-albedo, generally flat, and relatively rock-free surface. Within and around impact craters and fractures, laminated outcrop rocks with higher albedo are observed. Fine-grained materials include dark sand, bright ferric iron-rich dust, angular rock clasts, and millimeter-size spheroidal granules that are eroding out of the laminated rocks. Spectra of sand, clasts, and one dark plains rock are consistent with mafic silicates such as pyroxene and olivine. Spectra of both the spherules and the laminated outcrop materials indicate the presence of crystalline ferric oxides or oxyhydroxides. Atmospheric observations show a steady decline in dust opacity during the mission. Astronomical observations captured solar transits by Phobos and Deimos and time-lapse observations of sunsets.

Atmosphere↗
PubMed2004

Pancam multispectral imaging results from the Spirit Rover at Gusev Crater.

Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high- to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or hollows. Optically thick coatings of fine-grained ferric iron-rich dust dominate most bright soil and rock surfaces. Spectra of some darker rock surfaces and rock regions exposed by brushing or grinding show near-infrared spectral signatures consistent with the presence of mafic silicates such as pyroxene or olivine. Atmospheric observations show a steady decline in dust opacity during the mission, and astronomical observations captured solar transits by the martian moons, Phobos and Deimos, as well as a view of Earth from the martian surface.

Atmosphere↗
PubMed2004

Initial results from the Mini-TES experiment in Gusev Crater from the Spirit Rover.

The Miniature Thermal Emission Spectrometer (Mini-TES) on Spirit has studied the mineralogy and thermophysical properties at Gusev crater. Undisturbed soil spectra show evidence for minor carbonates and bound water. Rocks are olivinerich basalts with varying degrees of dust and other coatings. Dark-toned soils observed on disturbed surfaces may be derived from rocks and have derived mineralogy (+/-5 to 10%) of 45% pyroxene (20% Ca-rich pyroxene and 25% pigeonite), 40% sodic to intermediate plagioclase, and 15% olivine (forsterite 45% +/-5 to 10). Two spectrally distinct coatings are observed on rocks, a possible indicator of the interaction of water, rock, and airfall dust. Diurnal temperature data indicate particle sizes from 40 to 80 microm in hollows to approximately 0.5 to 3 mm in soils.

Carbonates↗
PubMed1997

Anatomy and embryology of the trigeminal nerve and its branches in the parasellar area.

The cavum trigeminale (Meckel's cave) anatomy is still poorly understood. Many different descriptions are found in the literature. In order to clarify the relationship of trigeminal ganglion and its branches with dura and arachnoid, we underwent an embryological and adult microanatomical and histological study. Serial sections of human embryos and fetuses were used. For adult study, microdissections and histological serial sections were performed. We found that dura and arachnoid stop at the trigeminal ganglion and do not extend the three branches of the trigeminal nerve. These three branches are embedded into separate peripheral sheaths. These results are important for clear understanding of the anatomy of the parasellar lodge (cavernous sinus) lateral wall.

Adult↗
PubMed1996

The venous system of the lateral sellar compartment (cavernous sinus): an histological and embryological study.

The microanatomy of the lateral sellar or parasellar venous system (so-called cavernous sinus) is poorly understood and is still passionately debated. The exact nature of this venous structure is not yet clear whether it is a plexus or a sinus. In order to understand the anatomy of this area better, an embryological and adult microanatomical study was performed. Serial histological sections of human embryos and fetuses of well determined ages (6, 7, 8, 10, 11, 12, 14, 30 weeks) were used. The adult study was performed with microdissections and serial histological sections of laterosellar compartments. The analysis of this material confirms that the parasellar venous system is a true sinus, on the embryological and histological point of view. They differ from true veins. As other dural sinuses, it may contain different types of channels: from simple venous canal to complex venous plexus. The opinions of different authors are reviewed in the introduction and discussed with the results.

Adult↗
PubMed1996

Endocrine neoplasia in New World primates.

Of 1,106 New World primates necropsied from the National Zoological Park (Washington, D.C.) and the Department of Comparative Pathology, Johns Hopkins University School of Medicine (Baltimore, Maryland) 22 (1.9%) animals were identified with 27 neoplasms. Of this group, nine animals (two females, seven males) had a total of 13 endocrine neoplasms. All animals were adults, with an age range of 2.7-25 years (average, 12.1 years). Seven were Callitrichidae and two were Cebidae. The adrenal gland was the most affected organ, with seven (53.8%) neoplasms, followed by the pituitary and thyroid gland with two (15.4%) cases each, and the pancreas and parathyroid gland with one tumor (7.7%) each. All neoplastic disorders were benign. Immunocytochemistry assays for growth hormone, adrenocorticotropic hormone, prolactin, follicle-stimulating hormone, luteinizing hormone, thyroid-stimulating hormone, and chromogranin A were performed on two pituitary neoplasms. Pheochromocytoma was the most frequent neoplasm, representing 5 (38.4%) of the 13 neoplasms. The remaining were thyroid cystadenoma (two, 15.4%), corticotrophic cell pituitary adenoma (two, 15.4%), adrenal ganglioneuroma (one, 7.7%), adrenal cortical adenoma (one, 7.7%), parathyroid chief-cell adenoma (one, 7.7%), and pancreatic islet-cell adenoma (one, 7.7%).

Adenoma↗
PubMed1993

Use and misuse of antibiotics in Latin America.

Some common characteristics that distinguish antibiotic use in Latin America are a high incidence of infections that are treatable with antibiotics, extensive use and frequent misuse of antibiotics, and frequent self-medication and nonprofessional prescription in the outpatient setting. Community-acquired organisms are generally more antibiotic-resistant in Latin America than in more-industrialized countries. Antibiotics also are used extensively in hospitals, largely for surgical prophylaxis and for nosocomial infections, which occur more frequently (in 15%-20%) in hospitalized patients. Prophylactic use of antibiotics is largely inappropriate--i.e., indiscriminate, inopportune, and prolonged. A frequent outcome of this inappropriate use is the occurrence of nosocomial infections due to strains that are much more drug resistant than those encountered in industrialized countries. The great number of pharmaceutical products available, and the lack of stringent policies regarding drug sales and advertising often result in pressure to prescribe and in confusion not only among the public at large but among physicians themselves. Coordinated efforts to educate health care professionals, campaigns against self-medication, stricter rules for drug sales and advertising, and restricted use of certain antibiotics in hospitals may contribute to rational antibiotic use.

Ambulatory Care↗
PubMedDate not supplied

Splenic abscesses due to Mycobacterium tuberculosis in patients with AIDS.

Among 60 patients with AIDS seen at our institution, two had splenic abscesses due to Mycobacterium tuberculosis without pulmonary tuberculosis. In both cases splenic abscess was the first manifestation of AIDS; the patients had prolonged fever and had lost weight and experienced malaise; slight hepatomegaly was noted in both instances and peripheral lymphadenopathy in one. Chest radiography gave normal results in one case and showed hilar lymphadenopathy in the other. Ultrasonographic findings were characteristic: homogeneous hepatomegaly and splenomegaly, with multiple filling defects of variable size. Diagnosis required splenectomy in one case and biopsy of cervical lymph nodes in the other. In both cases Ziehl-Neelsen staining gave positive results; M. tuberculosis grew from a culture of splenic tissue of one patient and from a culture of lymph nodal tissue of the other. There was a rapid response to antituberculous therapy. Splenic tuberculosis seems to be a distinct extrapulmonary entity in patients with AIDS. Ultrasonographic images are useful for diagnosis and follow-up.

Abscess↗