M96-1 for web

نویسنده

  • Donald K. Perovich
چکیده

Sea ice is a translucent material with an intricate structure and complex optical properties. Understanding the reflection, absorption, and transmission of shortwave radiation by sea ice is important to a diverse array of scientific problems, including those in ice thermodynamics and polar climatology. Radiative transfer in sea ice is a combination of absorption and scattering. Differences in the magnitude of sea ice optical properties are due primarily to differences in scattering. Spectral variations are mainly a result of absorption. Changes in such optical properties as the albedo, reflectance, transmittance, and extinction coefficient are directly related to changes in the state and structure of the ice. Physical changes that enhance scattering, such as the formation of air bubbles due to brine drainage, result in larger albedos and extinction coefficients. The albedo is quite sensitive to the surface state. If the ice has a snow cover, albedos are large. In contrast, the presence of liquid water on a bare ice surface causes a decrease in albedo, which is more pronounced at longer wavelengths. Sea-ice optical properties depend on the volume of brine and air and on how the brine and air are distributed. For conversion of SI units to non-SI units of measurement consult ASTM Standard E380-93, Standard Practice for Use of the International System of Units, published by the American Society for Testing and Materials, 1916 Race St., Philadelphia, Pa. 19103. Cover: Dr. T.C. Grenfell measuring melt pond albedos on first-year ice near Barrow, Alaska. A Kipp radiometer, which measures total shortwave irradiance, is in the foreground. The cylindrical instrument on the tripod is a scanning spectroradiometer that measures spectral irradiance from 400 to 2500 nm.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Effects of a kaolin-based particle film on obliquebanded leafroller (Lepidoptera: Tortricidae).

Studies were conducted in 1997 to evaluate the effects of the kaolin-based particle film formulation M96-018 on adults, eggs, and larvae of the obliquebanded leafroller, Choristoneura rosaceana (Harris). Particle film treatments significantly reduced female longevity, mating success, and number of egg masses oviposited compared with moths on untreated apple leaves in sleeve-cage and screen-cage...

متن کامل

Combinational Multiple-valued Circuit Design by Generalized Disjunctive Decomposition

1 This work has been supported in part by Found of Fundamental Investigations (Republic of Belarus), Grant ‹M96-094. Abstract A design of multiple-valued circuits based on the multiple-valued programmable logic arrays (MV PLA’s) by generalized disjunctive decomposition is presented. Main subjects are 1) Generalized disjunctive decomposition of multiple-valued functions using multiple-terminal m...

متن کامل

ar X iv : a st ro - p h / 01 04 04 9 v 1 3 A pr 2 00 1 1 56 CO γ - RAYS FROM SN 1998 BU : COMPTEL UPPER LIMITS

The type Ia supernova SN1998bu in M96 was observed by COMPTEL for a total of 88 days starting 17 days after the first detection of the supernova. The accumulated effective observation time was 4.14 Msec. The COMPTEL observations were performed in a special instrument mode improving the lowenergy sensitivity. We generated images in the 847 keV and 1238 keV lines of Co, using improved point sprea...

متن کامل

ar X iv : a st ro - p h / 99 02 05 6 v 1 3 F eb 1 99 9 INFRARED AND OPTICAL STUDY OF THE TYPE

The type Ia SN 1998bu was discovered in the galaxy M96 on 9 May 1998. It is one of the closest type Ia events of modern times and good temporal coverage has been achieved. Moreover its distance is well-determined. We describe here some of the first-season photometric and spectroscopic observations. While SN 1998bu is unusually highly reddened, we can still deduce that it was a typical type Ia e...

متن کامل

The Coma – Leo I Distance Ratio and the Hubble Constant

The diameter velocity dispersion relation in B, V, and K for three early type galaxies in the Leo I (M96) group is derived from published photometry and kinematic data. The relations in all three colors have slopes which agree well with those for the Coma cluster. The RMS scatter of the Leo I galaxies in each color is extremely small, consistent with the group’s compactness. These relations yie...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1996