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Article
Ink4a/Arf−/− and HRAS(G12V) transform mouse mammary cells into triple-negative breast cancer containing tumorigenic CD49f− quiescent cells
Intratumoral heterogeneity within individual breast tumors is a well-known phenomenon that may contribute to drug resistance. This heterogeneity is dependent on several factors, such as types of oncogenic driv...
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Article
Open AccessStatin use in primary inflammatory breast cancer: a cohort study
Some studies have suggested that statins, which have cholesterol-lowering and anti-inflammatory properties, may have antitumor effects. Effects of statins on inflammatory breast cancer (IBC) have never been st...
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Article
Ink4a and Arf are crucial factors in the determination of the cell of origin and the therapeutic sensitivity of Myc-induced mouse lymphoid tumor
The cell of origin of tumors and the factors determining the cell of origin remain unclear. In this study, a mouse model of precursor B acute lymphoblastic leukemia/lymphoma (pre-B ALL/LBL) was established by ...
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Chapter
Development of Millimeter-wave Radar for Latest Vehicle Systems
We developed the millimeter-wave radar that adopted both the FMpulse Doppler method and the Polarization-twisting Cassegrain antenna with mechanical scanning. Our radar features the following advantage: ▸ Wide...
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Article
The Hard X-ray Telescope (HXT) for the SOLAR-A mission
The Hard X-ray Telescope (HXT) is a Fourier-synthesis imager; a set of spatially-modulated photon count data are taken from 64 independent subcollimators and are Fourier-transformed into an image by using proc...
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Chapter
Microwave Observations of the Sun During the 22nd Solar Activity Cycle — 17 GHz Radio Heliograph
For the study of high energy phenomena on the Sun during the maximum period of the 22-nd solar activity cycle, we started to construct a radio heliograph at Nobeyama Radio Observatory. The operating frequency ...
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Chapter
The Hard X-ray Telescope (HXT) for the SOLAR-A Mission
The Hard X-ray Telescope (HXT) is a Fourier-synthesis imager; a set of spatially-modulated photon count data are taken from 64 independent subcollimators and are Fourier-transformed into an image by using proc...
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Article
Cytotoxic effects of a leukocidin from Fusobacterium necrophorum on bovine hepatic cells
Cytotoxic effects of a leukocidin from Fusobacterium necrophorum were demonstrated on bovine hepatic cells. The cytotoxic response was dose-dependent and could be inhibited by homologous antiserum. Scanning elect...
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Article
Radio evidence for a delayed acceleration process in solar flares
Evidence for a delayed acceleration process in solar flares is presented in the form of an analysis of simultaneous observations in microwaves, decimetre and metrewaves, and hard X-rays of six ‘delayed’ gradua...
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Article
X-ray imaging of a solar limb flare on 1982 January 22
Simultaneous X-ray images in hard (20–40 keV) and softer (6.5–15 keV) energy ranges were obtained with the hard X-ray telescope aboard the Hinotori spacecraft of an impulsive solar X-ray burst associated with ...
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Article
Can observed hard X-ray and microwave flux from solar flares be explained by a single electron population?
In attempting to explain observed hard X-ray and microwave flux from solar flares by a single population of energetic electrons, one has met a serious discrepancy of the order of 103–105 between the calculated an...
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Chapter
Can Observed Hard X-Ray and Microwave Flux from Solar Flares be Explained by a Single Electron Population?
In attempting to explain observed hard X-ray and microwave flux from solar flares by a single population of energetic electrons, one has met a serious discrepancy of the order of 103-105 between the calculated an...
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Article
Successive electron and ion accelerations in impulsive solar flares on 7 and 21 June 1980
A study of the relative timing of solar flare emissions at different wavelengths can provide valuable insights into the associated particle-acceleration mechanisms. We report here that the significant systemat...
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Article
Late phase gradual enhancements in microwaves and hard X-rays of the 6 November 1980 flare
Gradual enhancements which repeatedly appeared 20–50 min after the onset of an impulsive burst were observed in microwaves and hard X-rays. The observed characteristics of the gradual enhancements are (i) the ...
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Chapter and Conference Paper
Late Phase Gradual Enhancements in Microwaves and Hard X-rays of the 6 November 1980 Flare
Gradual enhancements which repeatedly appeared 20–50 min after the onset of an impulsive burst were observed in microwaves and hard X-rays. The observed characteristics of the gradual enhancements are (i) the ...
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Article
Source structure of gradual rise and fall bursts at 17 GHz
From ∼ 200 GRF (gradual rise and fall) bursts which have been recorded with the 17 GHz interferometer at Nobeyama, we deduce the following characteristics of GRF bursts: (1) Sources of GRF bursts are broader, ...
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Article
Coronal magnetic field structure derived from two-frequency radioheliograph observations
An exceptional variety of positions and polarizations was found for two type I storms and numerous sporadic bursts observed during 15 consecutive days with the Culgoora radioheliograph at 80 and 160 MHz. The r...
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Chapter
Coronal Magnetic Field Structure Derived from Two-Frequency Radioheliograph Observations
An exceptional variety of positions and polarizations was found for two type I storms and numerous sporadic bursts observed during 15 consecutive days with the Culgoora radio-heliograph at 80 and 160 MHz.
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Chapter
Unusual Absorption of a Solar Type II Burst by ‘Shadow’ Type III Bursts
The Hα-flare on 1968 August 23d23h45m was followed by a short-lived type II burst. The radio spectrograph record obtained at Culgoora is shown in Figure 1. The type II burst was of split-band structure with unusu...
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Article
The structure, polarization, and spatial relationship of solar radio sources of spectral types I and III
A description is given of recent high-resolution observations of the sun made at 80 MHz with the Culgoora radioheliograph. In many cases the sources of type I storms show bi-polar structure, the two components...
