我国个人信用征信制度中的隐私权保护

在我国个人信用征信制度中,个人征信机构的所有经营活动都是围绕着消费者的个人信用信息展开的。因此,不可避免的存在着侵犯消费者隐私权的情形,必须在确保个人征信业的健康发展与隐私权的保护之间寻找一个平衡点。在借鉴世界各国对隐私权保护的基础上,针对我国立法和司法对隐私权保护的不足,提出了我国在现阶段保护隐私权的一些设想。     

非古典正交多项式族{S_n~x(x)}的某些性质

本文对非古典正交多项式族{S_n~α(x)},提出它的估计以及展开定理。     

Efficiency of anthracene as a suspended scintillator for counting aqueous nickel-63 samples

Zusammenfassung Die Zählausbeute einer Anthrazenkristallsuspension als Szintillatormaterial wurde für die Betastrahlung des Ni-63-Isotops untersucht. Die Methode ist eine anpassungsfähige Ergänzung zur bekannten Flüssigkeitsszintillationsmessung.

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The authors are grateful to Dr.J. D. Punch of Medical College of Virginia for the use of his liquid scintillation spectrometer.     

The effects of acute and chronic morphine on regional distribution of cardiac output in brain

Summary Both acute and chronic administration of morphine resulted in an increase in the percent cardiac output received by brain. However, various brain regions were affected differently by the drug treatments. The greatest increases in percent cardiac output received after chronic administration of morphine occurred in pons and cerebellum, while the greatest increases after acute administration occurred in cortex and midbrain. The changes found are in contrast with earlier studies which suggest that morphine has no effect on cerebral blood flow.     

Supernova SN 2011fe from an exploding carbon-oxygen white dwarf star

Type Ia supernovae have been used empirically as 'standard candles' to demonstrate the acceleration of the expansion of the Universe even though fundamental details, such as the nature of their progenitor systems and how the stars explode, remain a mystery. There is consensus that a white dwarf star explodes after accreting matter in a binary system, but the secondary body could be anything from a main-sequence star to a red giant, or even another white dwarf. This uncertainty stems from the fact that no recent type Ia supernova has been discovered close enough to Earth to detect the stars before explosion. Here we report early observations of supernova SN 2011fe in the galaxy M101 at a distance from Earth of 6.4 megaparsecs. We find that the exploding star was probably a carbon-oxygen white dwarf, and from the lack of an early shock we conclude that the companion was probably a main-sequence star. Early spectroscopy shows high-velocity oxygen that slows rapidly, on a timescale of hours, and extensive mixing of newly synthesized intermediate-mass elements in the outermost layers of the supernova. A companion paper uses pre-explosion images to rule out luminous red giants and most helium stars as companions to the progenitor.