scholarly journals Determination of formaldehyde in fresh seafood under different washing and cooking conditions

2021 ◽  
Vol 6 (2) ◽  
pp. 158
Author(s):  
Pattama Senthong ◽  
Sivasit Wittayasilp ◽  
Tule Sirikitputtisak
Keyword(s):  
Cooking Conditions

Importance of Cooking Temperature and Pancreatic Amylase in Determination of Dietary Fiber in Dried Legumes

1995 ◽  
Vol 78 (6) ◽  
pp. 1444-1449 ◽  
Author(s):  
Roger Mongeau ◽  
René Brassard
Keyword(s):  
Dietary Fiber ◽  
Rapid Method ◽  
Dry Matter ◽  
Pancreatic Amylase ◽  
Total Dietary Fiber ◽  
Cooking Temperature ◽  
Navy Beans ◽  
Lima Beans ◽  
Cooking Conditions

Abstract Total dietary fiber (TDF) was measured in large lima, roman, black turtle, light red kidney, white navy, pinto, black-eyed, and soya beans and in chick peas by the Mongeau rapid method (A), the Prosky method (B), and the Lee method (C). When the samples were soaked and cooked according to package instructions (gentle boiling, 95°C), TDF values by method A were all within 19.7-22.1%, except for black-eyed beans (9.9%) and chick peas (11.3%) (g/100 g, cooked dry matter). For large lima beans (20.0-21.3%) and soya beans (19.2-19.7%), TDF values by methods A, B, and C were in agreement. For 7 samples, however, TDF values were up to 81% higher by method B (17.4-34.7%) and up to 122% higher by method C (21.1-39.8%) than those by method A (P ≤ 0.01). For 6 legumes, TDF values by method C were 15-28% higher (P ≤ 0.013) than by method B. White navy beans were analyzed also after different cooking conditions, varying from no cooking to autoclaving for 15 min at 120°C. TDF values by method A were independent from cooking conditions and remained between 20.2 and 22.4%. For navy beans cooked at 95°C, TDF values by method B (up to 34.7 ± 1.4%) and C (up to 39.8 ± 0.3%) were unpredictable, but autoclaving at 120°C reduced them to about 22%. Incorporation of a pan-creatic amylase in methods B and C consistently decreased the aforementioned analytical discrepancies, as did the absence of cooking. Only autoclaving (for at least 15 min at 120°C) fully restored agreement among methods A-C.

scholarly journals Determination of Furosine and Fluorescence as Markers of the Maillard Reaction for the Evaluation of Meat Products during Actual Cooking Conditions

2012 ◽  
Vol 18 (1) ◽  
pp. 67-76 ◽  
Author(s):  
Keiko YAMAGUCHI ◽  
Yuri NOMI ◽  
Takeshi HOMMA ◽  
Midori KASAI ◽  
Yuzuru OTSUKA
Keyword(s):  
Maillard Reaction ◽  
Meat Products ◽  
Cooking Conditions

scholarly journals Determination of Ideal Cooking Conditions for Pulp Production from Avocado Wood (Persea americana Mill.) by Kraft Method

2021 ◽  
Vol 72 (4) ◽  
pp. 411-416
Author(s):  
Gülşah Altunışık Bülbül ◽  
Ayhan Gençer
Keyword(s):  
Raw Materials ◽  
Persea Americana ◽  
Pulp Yield ◽  
Pulp Viscosity ◽  
Pulp Properties ◽  
Primary Basis ◽  
Pulp Production ◽  
Cooking Conditions ◽  
The Ideal

In this study, hand sheets were made from pulp produced by the Kraft method using avocado wood. The raw materials were supplied by a fruit orchard and consisted of avocado (Persea americana Mill.) trees that had completed their useful life and were cut during routine thinning maintenance. In order to determine the ideal cooking conditions in the production of pulp from avocado wood via the Kraft method, 16 cooks were carried out by varying the cooking time (T), active alkali (AA), and sulfidity (S) ratios. The general pulp properties, especially the screened pulp yield, pulp viscosity, and Kappa number, were evaluated. The pulp yield was taken as the primary basis in determining the cooking conditions. The ideal cooking conditions were also determined by considering some physical, mechanical, and optical properties of the paper. According to this study, the conditions found to be ideal in pulp production from avocado (Persea americana Mill.) wood via the Kraft method were: 18 % AA, 22 % S, and 75 min T.

Determination of perfluorooctanoic acid (PFOA) extractable from the surface of commercial cookware under simulated cooking conditions by LC/MS/MS

The Analyst ◽  
2005 ◽  
Vol 130 (9) ◽  
pp. 1299 ◽  
Author(s):  
Charles R. Powley ◽  
Michael J. Michalczyk ◽  
Mary A. Kaiser ◽  
L. William Buxton
Keyword(s):  
Perfluorooctanoic Acid ◽  
Cooking Conditions

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.

Distance to SN 1987A and the LMC

1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia
Keyword(s):  
Angular Size ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Light Curves ◽  
Distance Modulus ◽  
Absolute Size ◽  
Sn 1987A

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.

International determination of the total motion of the pole

1961 ◽  
Vol 13 ◽  
pp. 29-41
Author(s):  
Wm. Markowitz
Keyword(s):  
Secular Motion ◽  
The Future

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).

Time and Latitude in South Africa

1972 ◽  
Vol 1 ◽  
pp. 27-38
Author(s):  
J. Hers
Keyword(s):  
South Africa ◽  
Cape Town ◽  
Astronomical Observations ◽  
Royal Observatory ◽  
The Republic ◽  
Astronomical Determination ◽  
Limited Accuracy ◽  
Better Than

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.

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