The Action of Radium and X Rays on Malignant Cells

1921 ◽  
Vol 25 (11) ◽  
pp. 346-352
Author(s):  
J. H. Douglas Webster
Keyword(s):  
X Rays ◽  
2003 ◽  
Vol 131 (11-12) ◽  
pp. 458-460 ◽  
Author(s):  
Olivera Markovic ◽  
Dragomir Marisavljevic ◽  
Vesna Cemerikic-Martinovic

Nodal presentation of Burkitt-like lymphoma is common, particularly in gastrointestinal tract. However, only few cases with massive ascites and signs of subileus due to lymphoma proliferation are described. We report a 31-year-old male patient who presented with fever, night sweats, vomiting and abdominal fullness. Physical examination suggested much ascites. Abdominal X-rays showed hidroaeric levels. Diagnosis of Burkitt-like lymphoma was established on the basis of cytological and imunohistochemical examination of ascites (immune phenotype of malignant cells was EMA -, NSE -, LCA +, CD10 -/+, CD20 +, IgM +, Ki-67 +100%). After treatment with BMF protocol complete remission was achieved and retained for 2.5 years. Authors stressed that imunohistochemical examination of ascites has been proved as simple and efficient method for establishing precise diagnosis. In this way laparotomy was avoided, which otherwise would be necessary due to exclusive abdominal localization of the disease.


There are many considerations in the successful treatment of a tumour in the animal body by radiation. Broadly speaking, the subject may be divided into two main divisions : (1) the action of X-rays and the beta- and gamma-rays from radium on the tumour cells, and (2) the effect of these rays upon the animal itself. In both cases a gradual change of effects is observed according to the dose of radiation. Actively growing malignant cells, given a large dose of radiation, degenerate and die when re-inoculated into a living animal ; a dose short of this quantity causes the tumour cells to grow at a slower rate than they would do normally, but if given a very small dose, the cells appear to be stimulated rather than hindered in their subsequent growth.


2012 ◽  
Vol 65 (1-2) ◽  
pp. 5-8
Author(s):  
Aleksandra Lovrenski ◽  
Milana Panjkovic ◽  
Dragana Tegeltija ◽  
Ljiljana Tadic-Latinovic ◽  
Jelena Krcedinac

Malignant mesothelioma is the most significant pleural tumour and it can be divided into three types: epithelial, sarcomatoid and biphasic mesothelioma. The most significant clinical manifestation of this tumour is pleural effusion. This paper was aimed at determining the role of cytological evaluation of pleural fluid in the diagnosis of malignant mesothelioma. This retrospective study included 33 medical records of patients with pleural malignant mesothelioma referred to the Institute for Lung Diseases of Vojvodina, in Sremska Kamenica in the period from 2004 to 2009. In 24 out of 33 patients, x-rays confirmed pleural effusion, thoracentesis was performed and specimens of effusion were cytologically examined at the Department of Pathology of the Institute for Lung Diseases of Vojvodina. Forty-nine cytological examinations were done. Only 2 of the first specimens were positive for malignant cells and 6 were suspicious. In repeated cytological examinations, 5 out of 6 initially suspicious specimens were positive for malignant cells, and the remaining 1 was negative. To sum up, 7 of 49 cytological examinations were positive and the sensitivity of our cytological study for the diagnosis of malignancy was 29%. Due to the low sensitivity of the cytological examinations, it has been recommended to perform biopsy of the pleura for definitive diagnosis in every patient with clinical symptoms and suspicious radiography.


1994 ◽  
Vol 144 ◽  
pp. 82
Author(s):  
E. Hildner

AbstractOver the last twenty years, orbiting coronagraphs have vastly increased the amount of observational material for the whitelight corona. Spanning almost two solar cycles, and augmented by ground-based K-coronameter, emission-line, and eclipse observations, these data allow us to assess,inter alia: the typical and atypical behavior of the corona; how the corona evolves on time scales from minutes to a decade; and (in some respects) the relation between photospheric, coronal, and interplanetary features. This talk will review recent results on these three topics. A remark or two will attempt to relate the whitelight corona between 1.5 and 6 R⊙to the corona seen at lower altitudes in soft X-rays (e.g., with Yohkoh). The whitelight emission depends only on integrated electron density independent of temperature, whereas the soft X-ray emission depends upon the integral of electron density squared times a temperature function. The properties of coronal mass ejections (CMEs) will be reviewed briefly and their relationships to other solar and interplanetary phenomena will be noted.


2000 ◽  
Vol 179 ◽  
pp. 263-264
Author(s):  
K. Sundara Raman ◽  
K. B. Ramesh ◽  
R. Selvendran ◽  
P. S. M. Aleem ◽  
K. M. Hiremath

Extended AbstractWe have examined the morphological properties of a sigmoid associated with an SXR (soft X-ray) flare. The sigmoid is cospatial with the EUV (extreme ultra violet) images and in the optical part lies along an S-shaped Hαfilament. The photoheliogram shows flux emergence within an existingδtype sunspot which has caused the rotation of the umbrae giving rise to the sigmoidal brightening.It is now widely accepted that flares derive their energy from the magnetic fields of the active regions and coronal levels are considered to be the flare sites. But still a satisfactory understanding of the flare processes has not been achieved because of the difficulties encountered to predict and estimate the probability of flare eruptions. The convection flows and vortices below the photosphere transport and concentrate magnetic field, which subsequently appear as active regions in the photosphere (Rust & Kumar 1994 and the references therein). Successive emergence of magnetic flux, twist the field, creating flare productive magnetic shear and has been studied by many authors (Sundara Ramanet al.1998 and the references therein). Hence, it is considered that the flare is powered by the energy stored in the twisted magnetic flux tubes (Kurokawa 1996 and the references therein). Rust & Kumar (1996) named the S-shaped bright coronal loops that appear in soft X-rays as ‘Sigmoids’ and concluded that this S-shaped distortion is due to the twist developed in the magnetic field lines. These transient sigmoidal features tell a great deal about unstable coronal magnetic fields, as these regions are more likely to be eruptive (Canfieldet al.1999). As the magnetic fields of the active regions are deep rooted in the Sun, the twist developed in the subphotospheric flux tube penetrates the photosphere and extends in to the corona. Thus, it is essentially favourable for the subphotospheric twist to unwind the twist and transmit it through the photosphere to the corona. Therefore, it becomes essential to make complete observational descriptions of a flare from the magnetic field changes that are taking place in different atmospheric levels of the Sun, to pin down the energy storage and conversion process that trigger the flare phenomena.


Author(s):  
R. F. Bils ◽  
W. F. Diller ◽  
F. Huth

Phosgene still plays an important role as a toxic substance in the chemical industry. Thiess (1968) recently reported observations on numerous cases of phosgene poisoning. A serious difficulty in the clinical handling of phosgene poisoning cases is a relatively long latent period, up to 12 hours, with no obvious signs of severity. At about 12 hours heavy lung edema appears suddenly, however changes can be seen in routine X-rays taken after only a few hours' exposure (Diller et al., 1969). This study was undertaken to correlate these early changes seen by the roengenologist with morphological alterations in the lungs seen in the'light and electron microscopes.Forty-two adult male and female Beagle dogs were selected for these exposure experiments. Treated animals were exposed to 94.5-107-5 ppm phosgene for 10 min. in a 15 m3 chamber. Roentgenograms were made of the thorax of each animal before and after exposure, up to 24 hrs.


Author(s):  
R. H. Duff

A material irradiated with electrons emits x-rays having energies characteristic of the elements present. Chemical combination between elements results in a small shift of the peak energies of these characteristic x-rays because chemical bonds between different elements have different energies. The energy differences of the characteristic x-rays resulting from valence electron transitions can be used to identify the chemical species present and to obtain information about the chemical bond itself. Although these peak-energy shifts have been well known for a number of years, their use for chemical-species identification in small volumes of material was not realized until the development of the electron microprobe.


Author(s):  
E. A. Kenik ◽  
J. Bentley

Cliff and Lorimer (1) have proposed a simple approach to thin foil x-ray analy sis based on the ratio of x-ray peak intensities. However, there are several experimental pitfalls which must be recognized in obtaining the desired x-ray intensities. Undesirable x-ray induced fluorescence of the specimen can result from various mechanisms and leads to x-ray intensities not characteristic of electron excitation and further results in incorrect intensity ratios.In measuring the x-ray intensity ratio for NiAl as a function of foil thickness, Zaluzec and Fraser (2) found the ratio was not constant for thicknesses where absorption could be neglected. They demonstrated that this effect originated from x-ray induced fluorescence by blocking the beam with lead foil. The primary x-rays arise in the illumination system and result in varying intensity ratios and a finite x-ray spectrum even when the specimen is not intercepting the electron beam, an ‘in-hole’ spectrum. We have developed a second technique for detecting x-ray induced fluorescence based on the magnitude of the ‘in-hole’ spectrum with different filament emission currents and condenser apertures.


Author(s):  
C.W. Akey ◽  
M. Szalay ◽  
S.J. Edelstein

Three methods of obtaining 20 Å resolution in sectioned protein crystals have recently been described. They include tannic acid fixation, low temperature embedding and grid sectioning. To be useful for 3-dimensional reconstruction thin sections must possess suitable resolution, structural fidelity and a known contrast. Tannic acid fixation appears to satisfy the above criteria based on studies of crystals of Pseudomonas cytochrome oxidase, orthorhombic beef liver catalase and beef heart F1-ATPase. In order to develop methods with general applicability, we have concentrated our efforts on a trigonal modification of catalase which routinely demonstrated a resolution of 40 Å. The catalase system is particularly useful since a comparison with the structure recently solved with x-rays will permit evaluation of the accuracy of 3-D reconstructions of sectioned crystals.Initially, we re-evaluated the packing of trigonal catalase crystals studied by Longley. Images of the (001) plane are of particular interest since they give a projection down the 31-screw axis in space group P3121. Images obtained by the method of Longley or by tannic acid fixation are negatively contrasted since control experiments with orthorhombic catalase plates yield negatively stained specimens with conditions used for the larger trigonal crystals.


Author(s):  
C. W. Mehard ◽  
W. L. Epstein

The underlying cause of a disease may not he readily apparent but may have a long history in development. We report one such case which was diagnosed with the aid of the analytical electron microscope.The patient, a 48 yr. old white female, developed a tender nodule on the sole of her foot in December, 1981. Subsequently additional lesions developed on the same foot resulting in deep pain and tenderness. Superficial lesions also extended up to the knee on both legs. No abnormalities were revealed in blood tests or chest X-rays.


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